The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, surrounded by a more diffuse halo or extended envelope. The color profile suggests a predominantly older stellar population, indicated by the yellowish-orange hue. There is little evidence of significant dust lanes or active star formation regions based on the data, although there might be a low level present. The galaxy appears relatively undisturbed, showing no signs of recent major mergers or tidal interactions. It seems to be an evolved system nearing the red sequence with little star formation.
