The galaxy presents as a single, concentrated luminosity. It exhibits a generally elliptical morphology, appearing largely spheroidal rather than disc-like, with an approximate effective radius of 3.8 kpc. The light profile is smooth and centralized, suggesting a high degree of symmetry. The main body shows a dominant golden hue. There is a very weak hint of a less intense, redder outer envelope extending away from the central region. No spiral arm structure or distinct features are discernible. The morphology and color suggest a galaxy dominated by an older stellar population, possibly with ongoing star formation. There is a very slight asymmetry in the light distribution, with the upper right portion being slightly more extended. There are faint hints of disturbance but this is not well defined in the image. Overall, this is likely a massive galaxy.
