The galaxy presents as a relatively smooth, centrally concentrated object with a pronounced reddish-orange hue, suggesting a population dominated by older stars. The morphology appears elliptical or lenticular due to the lack of clearly defined spiral arms or a prominent disk structure. There is some evidence of a possible interaction or merger event, indicated by subtle distortions in the outer regions of the galaxy, but it appears to be a minor disturbance at most. The overall roundness of the galaxy is notable, further suggesting a lack of significant rotational structure.
