The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a concentrated central region, with a gradual decrease in luminosity outward. The core appears bright and yellowish, possibly indicating an older stellar population and diminished star formation activity.

There is faint evidence of some structural features, but it is difficult to ascertain distinct spiral arms or a well-defined disk. There are hints of some minor disturbances in the overall shape, possibly indicating a past or ongoing minor interaction. However, overall the galaxy does not show any distinct signs of a significant major merger or tidal disruption. The light distribution appears relatively uniform and symmetrically round.
