The galaxy presents as a relatively smooth, centrally concentrated object with a moderate ellipticity. The central region exhibits a yellow-white hue, possibly indicative of an older stellar population. The outer regions display a subtle blue tint, which may suggest the presence of some younger stars, and therefore ongoing or recent star formation, but at a modest rate. There is some visual evidence of a very faint disk, but the galaxy appears mostly spheroidal. There is the suggestion of possible tidal disturbance or minor interaction with another object in the lower left quadrant. The overall impression is of a galaxy transitioning to a more quiescent state.
