The galaxy presents as a disk galaxy, viewed at a significant angle, approaching edge-on. The central bulge is prominent and exhibits a smooth, concentrated light profile, appearing yellowish in color, suggestive of an older stellar population. The disk component, extending outward from the bulge, appears bluer, hinting at ongoing or recent star formation. The disk appears somewhat disturbed or patchy with areas that are not smoothly connected. There are no apparent signs of a major ongoing merger. Faint disturbances can be seen in the outer edges of the disk indicating a possible minor merger in the recent past. Overall the galaxy has a concentrated profile.
