The galaxy presents as an elliptical or lenticular morphology. It exhibits a generally smooth appearance, lacking prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, suggesting a significant bulge component. The galaxy is not perfectly circular but appears somewhat elongated, with a ratio of the major to minor axes suggestive of an E4-E5 elliptical type. There may be some minor asymmetry or a faint tidal feature. The overall color appears reddish-yellow, indicating an older stellar population with relatively low current star formation activity. This color suggests that the galaxy is primarily composed of evolved stars, with a minimal contribution from young, hot stars that would produce a bluer color. Overall the shape of the galaxy is somewhere between a perfect circle and a cigar shape. There are no signs of any major galaxy mergers. There is no indication of any minor disturbances.
