The galaxy presents as a largely smooth, elliptical structure with a cigar-like elongation. There is a pronounced central bulge exhibiting a yellowish-white hue, indicative of an older stellar population. This core region is surrounded by a fainter, more diffuse halo. A hint of bluer light is present on one side, which could possibly indicate minor ongoing star formation within a disk-like component, or the tail of a merger event. The overall morphology suggests that the galaxy is relatively undisturbed, with no signs of recent major mergers or tidal disruptions. The galaxy is relatively massive with a moderate rate of star formation.
