The galaxy presents as a somewhat elliptical, smooth object with a noticeable central bulge. The light distribution appears concentrated towards the center, with a gradual decrease in surface brightness towards the outer regions. The color profile indicates a redder core, likely indicative of an older stellar population, and bluer, albeit faint, extensions on the periphery that suggest possible regions of recent star formation. There is a faint, elongated feature to the left, which could indicate tidal disturbances or a companion galaxy, though further observation is necessary to confirm this. Overall, the galaxy exhibits characteristics consistent with an early-type spiral galaxy, or a lenticular galaxy undergoing some form of minor interaction.
