The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a high density of stars and possibly an active galactic nucleus, though this cannot be confirmed from the available image. Moving outward from the core, the light gradually decreases, creating a smooth luminosity profile with no evident spiral arm structure or distinct features. There is a lack of discernible dust lanes or prominent star-forming regions. The overall color appears to be yellowish-red. There appears to be a slight asymmetry with a more luminous area to the upper right of the core. The outer regions are diffuse, and there is no readily apparent interaction with any other galaxy or tidal debris present.
