The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge that appears bright and featureless, indicating a high density of stars. The galaxy's overall shape is somewhat elongated, with a cigar-like form. There is a slight indication of a disc, though it is less prominent than in spiral galaxies. The lack of strong spiral arms and the overall smooth light distribution suggest that the galaxy is likely dominated by an older stellar population. The central region could harbor a supermassive black hole, but this is only speculative. Based on its morphology, it is likely undergoing a relatively low rate of star formation. There may be some evidence of a minor disturbance in the overall shape but it may be due to minor interaction with another galaxy.
