The galaxy presents a moderately bright profile, exhibiting a concentrated central bulge that graduates into a less defined, more diffuse halo. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population, while the fainter halo displays a bluer tint, potentially indicative of ongoing star formation. The overall shape approximates a flattened spheroid, with a slight elongation that might hint at a minor distortion or interaction. There may be a slight irregularity in its overall symmetry, which could possibly be due to a small disturbance.
