The galaxy presents a diffuse, somewhat irregular morphology, exhibiting a moderate degree of internal structure. Its overall color appears bluish, suggesting the presence of a relatively young stellar population and ongoing star formation. The galaxy lacks a well-defined central bulge or nucleus, and the light is distributed in a clumpy, uneven manner. Faint, disturbed features are present, potentially indicating a past or ongoing interaction or merger event. The galaxy's shape is moderately elliptical, though its edges are not sharply defined, fading gradually into the background. There are indications of disruption and tidal features. Overall, the galaxy appears to be a dynamically active system undergoing significant evolutionary processes.
