This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades towards the outer edges. The overall color appears to be slightly redder, possibly indicating an older stellar population and diminished star formation activity. There are no prominent spiral arms or distinct features visible, although there appears to be a slight asymmetry in the outer halo. The galaxy seems relatively isolated, showing no signs of major mergers or strong tidal interactions with neighboring galaxies, though the possible hint of disturbance cannot be ruled out.
