This galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears quite concentrated towards the center, suggesting an older stellar population and minimal ongoing star formation. There's little evidence of spiral arms or a prominent disk structure; rather, it appears as a largely spheroidal system. No significant dust lanes or tidal features are discernible, which supports that the galaxy is relatively undisturbed. The color appears consistent with a redder galaxy, corroborating the suggestion of an older stellar population. Overall, the galaxy gives the impression of a passively evolving system without current or recent major merger activity.
