The galaxy presents as a somewhat elliptical, centrally concentrated object. There is a dominant, bright central bulge that appears smooth and yellowish-white in color, indicating an older stellar population. Surrounding the bulge is a fainter, more diffuse halo. There is only slight evidence of a disk structure. The halo exhibits a bluer hue. There are no prominent spiral arms, bar features, or significant dust lanes visible. The galaxy shows no strong evidence of any major ongoing merger activity or tidal disturbances. It's fairly rounded with no obvious extensions or distortions. The color gradient suggests ongoing star formation, albeit at a modest rate, primarily in the outer regions. Overall, the galaxy appears to be a relatively evolved system, likely an early-type spiral or elliptical.
