The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity towards the outer regions. The galaxy displays a yellowish-white hue, suggestive of an older stellar population dominating the light output. The overall morphology indicates a spheroid-dominated system. There's no obvious presence of spiral arms or a distinct disk component. The galaxy appears undisturbed, without any significant signs of ongoing mergers or tidal interactions. Its shape is approximately round, showing no signs of significant elongation or asymmetry.
