The galaxy presents as a single, concentrated object with a relatively smooth light distribution. It exhibits a generally elliptical morphology, appearing nearly circular on the sky. The core is bright and yellowish, with the light intensity gradually decreasing towards the outer edges. There is a subtle color gradient visible, shifting towards slightly bluer hues in the outer regions, though overall the galaxy appears to be primarily composed of older stellar populations. The structure lacks any obvious spiral arms, bars, or other distinct features. There is no clear indication of any major ongoing merging events or significant tidal disturbances, although the presence of subtle, minor disturbances cannot be completely ruled out.
