The galaxy presents a relatively smooth morphology with a centrally concentrated light profile. It appears elliptical or lenticular when viewed from our line of sight. The core of the galaxy exhibits a yellowish-orange hue, suggesting an older stellar population is dominant. The outer regions display bluer tones, suggestive of the presence of some younger stars or ongoing, albeit low, star formation. There is no readily apparent spiral structure. It appears undisturbed with no signs of recent major mergers, though some minor asymmetry in the outer regions suggests potential past interaction or accretion events.
