The galaxy presents as a primarily smooth, elliptical structure with a concentrated central bulge. Its overall color profile suggests a population of older stars, contributing to a yellowish hue in the core region. A fainter, bluer disk-like component is observed surrounding the central bulge, hinting at more recent star formation activity, albeit at a lower rate. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated along a particular axis. There is some subtle evidence of minor tidal disturbances or asymmetries in the outer regions, possibly indicating past or ongoing interactions with nearby galaxies.
