The galaxy presents as an elongated, elliptical structure. A concentrated central bulge exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a bluer tint, possibly indicating younger stars. The overall morphology is smooth, lacking significant spiral arm features or prominent dust lanes. There may be some subtle distortion in the galaxy's shape, which could imply a past interaction or minor disturbance. The galaxy appears relatively isolated with no obvious companion galaxies in close proximity.
