The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal with a concentrated central bulge. There is a distinct color gradient, shifting from a yellowish-orange core region towards bluer hues in the outer edges. The overall color suggests an older stellar population, although bluer regions potentially indicate some ongoing, albeit subdued, star formation. There is no apparent spiral structure or evidence of significant dust lanes within the galaxy. The light distribution appears relatively uniform with no pronounced tidal features or signs of recent major mergers, though subtle disturbances cannot be entirely ruled out. Based on its round shape and color profile, it appears to be a relatively evolved system.
