The galaxy presents as a somewhat elliptical structure with a concentrated central bulge that emits strongly. The core appears yellow in color, suggestive of an older stellar population. Surrounding the bulge, a more diffuse halo is observed, with a bluer hue indicating more recent star formation, although this activity appears to be relatively subdued. The galaxy's edges are not sharply defined, but gradually fade into the background, implying a smooth distribution of stars and gas in the outer regions. There is no obvious disk or spiral structure visible. Some minor irregularities in the outer halo might suggest a past interaction or minor disturbance, but overall, the galaxy exhibits a fairly relaxed morphology.
