The galaxy presents as a relatively smooth, lenticular structure. The overall shape appears to be elliptical, with the ratio of major to minor axes suggesting a moderate degree of flattening. The light is concentrated towards the center. There is some indication of a disk-like structure. There are faint hints of spiral structure, as well as an indication of minor disturbance. Colors suggest the presence of both older stellar populations and a low level of ongoing star formation. The galaxy shows a red central bulge, surrounded by blue colors, particularly toward the edge of the disk, indicating areas with ongoing star formation. There is no clear evidence of a major merger or significant tidal interactions.
