The galaxy appears as a relatively smooth, elliptical or lenticular structure. Its light profile suggests a centrally concentrated bulge that dominates the galaxy's luminosity. The galaxy appears mostly homogenous, with little indication of spiral arms or significant dust lanes. The light distribution is nearly circular, indicating that it is likely viewed face-on or with a small inclination. There is a slight color gradient, with a more yellow hue towards the center, possibly indicating an older stellar population concentrated in the galactic bulge. The outer regions appear somewhat bluer, which is consistent with the presence of a younger stellar population. There is no significant evidence of an active galactic nucleus, nor is there any indication of a recent major merger event or tidal disturbances. The image suggests this is a galaxy with little ongoing star formation.
