The galaxy appears to be an elliptical type, exhibiting a smooth, spheroidal morphology. It displays a centrally concentrated luminosity profile. The central region exhibits a yellow-gold hue, indicative of an older stellar population. Moving outwards from the core, the color becomes slightly bluer, suggesting the presence of some younger stars. A slight elongation is present, indicating a deviation from a perfectly spherical shape. There may be some minor tidal disturbances, as the outer edges are slightly irregular. The galaxy appears to be relatively isolated, without any clear signs of a major merger event. The overall color suggests a galaxy with ongoing, but not vigorous, star formation.
