The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a decreasing gradient in luminosity outward. The color profile suggests an older stellar population, trending towards redder hues. There is little evidence of spiral arm structure, distinct dust lanes, or active star formation regions. The overall form appears relatively undisturbed, lacking any strong indication of recent or ongoing major merger activity, though there may be a minor visual disturbance to the upper left that could possibly be tidal debris. The galaxy is largely spheroidal in appearance with a generally rounded shape.
