The galaxy presents as a somewhat elliptical, disk-like structure with a notable central bulge. The color profile suggests a population of older stars, contributing to a reddish-yellow hue that is most pronounced near the center. There appears to be a smooth morphology, with a lack of prominent spiral arms or significant dust lanes. A slight elongation is observed, deviating from a perfectly circular shape and tending towards a cigar-like structure. There is no readily apparent visual evidence of major mergers or strong tidal disturbances affecting the galaxy's overall structure. Faint, blue-tinged regions may indicate pockets of recent or ongoing star formation, although these features are not dominant.
