The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated luminosity profile indicative of a large spheroidal component. The core region displays a high surface brightness, appearing almost uniformly bright with a yellow-white color, suggesting a high density of older stellar populations. Moving outward from the core, the galaxy's light gradually fades into the surrounding sky. The outer regions appear somewhat diffuse and possess a reddish hue, potentially indicating a population of older, redder stars and/or the presence of dust obscuration. There is no discernible spiral arm structure or distinct features to suggest recent or ongoing major star formation. A slight asymmetry might be present, but it is unclear whether this is intrinsic to the galaxy or due to observational effects.
