The galaxy presents as a slightly elongated, disk-shaped object. It appears to have a prominent central bulge that emits strongly in what seems to be yellow light, suggestive of an older stellar population. A fainter disk surrounds the bulge. The light distribution appears relatively smooth, with hints of spiral arm structure but not well defined. There are color gradients across the disk with one region possibly indicating recent star formation. There is very little evidence of tidal disturbances, suggesting the galaxy has not undergone a recent major merger. It appears to be a galaxy that is not perfectly smooth, but with relatively undisturbed morphology, and which may be undergoing moderate star formation.
