The galaxy presents a morphology indicative of an elliptical or lenticular type. It exhibits a relatively smooth, concentrated light profile, with a central bulge region that appears nearly spherical. There is very little evidence of spiral arm structure or significant dust lanes. The color is predominantly yellowish-orange, suggesting a population of older stars and a lower rate of on-going star formation. A slight disturbance or tidal feature may be present on one side of the galaxy, hinting at a possible past interaction with another galaxy, however, the possibility of a recent merger appears to be low.
