The galaxy presents as a generally smooth, elliptical-like structure. There is a concentrated central bulge which exhibits a yellowish hue, suggesting an older stellar population. A surrounding disk is present, exhibiting a bluer hue, suggestive of more recent or ongoing star formation, although at a relatively low rate. The galaxy appears generally undisturbed with no signs of major mergers or tidal interactions. The overall morphology is broadly consistent with an early-type galaxy.
