The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge dominates the galaxy's structure. This suggests an older stellar population residing within the core. There is a subtle, diffuse halo extending outwards from the core, decreasing in intensity with distance. The overall color appears to be relatively uniform across the galaxy. There is no significant evidence of spiral arm structure or dust lanes. The light distribution is consistent with an early-type galaxy, possibly an elliptical or lenticular system. Slight elongation can be observed, implying that it is not perfectly round. There is no significant evidence of recent major merger activity. 
