The galaxy appears as a roughly elliptical, centrally concentrated object. It exhibits a smooth morphology with a significant fraction of its light concentrated in a bright, unresolved core. There is little evidence of spiral arm structure or strong morphological disturbances. The light profile gradually fades from the central core outwards into a more diffuse halo. The color appears to be a blend of blue and red, with a slightly yellower central region and bluer outer regions. This color gradient could indicate a radial variation in stellar populations, with older, redder stars concentrated in the core, and younger, bluer stars in the outer regions. There is some indication of minor asymmetric features in the halo, suggesting possible tidal interactions or past mergers, though these are subtle. Overall, the galaxy appears to be a relatively evolved system with moderate star formation activity.
