The galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated shape. It displays a prominent central bulge that gradually fades into a more diffuse halo. The core of the galaxy exhibits a yellowish-orange hue, potentially indicating an older stellar population. The outer regions of the galaxy show a bluer tint, possibly suggesting the presence of some younger stars, although the overall star formation rate appears to be low. There's a very slight hint of a possible disk component, but it is not prominent. There is no strong evidence of any significant tidal disturbances or ongoing major merging events. The galaxy's color profile is somewhat uniform, with only subtle color variations observed between the core and the outer regions.
