The galaxy presents as a moderately inclined, disk-shaped system. The central bulge is pronounced, exhibiting a smooth, concentrated light profile with a yellowish-orange hue, indicative of an older stellar population. Moving outward from the bulge, the disk appears relatively smooth with some faint, diffuse blue regions on the left side. The overall shape is somewhere between round and cigar shaped. There appears to be some sort of minor disturbance in the disk, but no clear merging activity is evident.
