The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing elongated but without a pronounced disk structure. Color gradients are subtle, with a yellowish core transitioning to slightly redder outer regions. No distinct spiral arm features or prominent dust lanes are discernible. The overall appearance suggests a lack of significant recent or ongoing star formation, consistent with an older stellar population. There is some evidence of minor disturbance of the galaxy, though it appears to be a fairly relaxed system.
