This galaxy appears as a moderately bright object with a redshift of approximately 0.43, suggesting it is located at a considerable distance. It presents a somewhat irregular morphology, appearing neither perfectly elliptical nor clearly spiral. The main body of the galaxy exhibits a diffuse, yellowish-orange glow, potentially indicating an older stellar population and a lack of significant ongoing star formation in the central regions.

There is some indication of disturbed morphology, with hints of possible tidal features or ongoing merger activity. Some asymmetry in the light distribution suggests a departure from a relaxed, equilibrium state. This galaxy does not appear to possess a well-defined disk or prominent spiral arms. The color indices suggest relatively redder colors, which could correspond to a population dominated by older stars.

Overall, this galaxy seems to be an intermediate mass system undergoing some form of dynamical interaction or disturbance, and/or has had it's star formation quenched. The relatively high redshift makes detailed morphological analysis challenging. Further high-resolution imaging and spectroscopic observations would be needed to better understand the nature and evolutionary state of this system.
