This galaxy presents as an elliptical or lenticular type. Its light distribution appears relatively smooth with a high degree of central concentration, though there are indications of subtle structural features that might be a disk. The overall shape is elongated and cigar shaped, suggestive of some triaxiality. There are no obvious spiral arms or strong dust lanes visible. The central region exhibits a brighter, slightly bluer tint compared to the outer regions, indicating potential ongoing, low-level star formation. It is not interacting with any neighboring galaxies, although there seems to be a disturbance occurring in the lower quadrant.
