The galaxy presents as a somewhat elongated, disk-like structure. It exhibits a central bulge that appears yellowish-white, possibly indicating a population of older stars. The outer regions of the disk are subtly bluer, which may suggest ongoing star formation in these areas. The galaxy's overall morphology appears relatively smooth, but with some indication of spiral arms or a disk-like structure. The galaxy's shape is more cigar-shaped than round. There is no obvious evidence of a major merger or significant tidal disturbances; its structure appears relatively unperturbed. There may be evidence of some minor disturbance or asymmetry. The galaxy's size, based on the scale, suggests it is a moderate-sized galaxy.
