The galaxy presents as a somewhat diffuse object with a central concentration of light, suggesting the presence of a bulge or a centrally located active galactic nucleus. The overall shape is largely smooth and elliptical, though some subtle irregularities may be present. There is a faint hint of spiral structure or perhaps some tidal disturbances, but the image resolution makes it difficult to discern definitively. The galaxy exhibits a blueish hue, indicative of ongoing star formation or a younger stellar population. Based on the color and luminosity, this galaxy is likely a moderately massive system undergoing a moderate amount of star formation. There is some indication of a possible minor disturbance in the outer regions, but it is not conclusive evidence of a merger.
