The galaxy presents as a centrally concentrated object with a largely smooth morphology. The central region exhibits a yellowish hue, potentially indicating an older stellar population. Fainter greenish colors surrounding the central region suggest the presence of some star formation, albeit relatively low. The overall shape appears nearly circular, showing little disk structure. There are hints of minor asymmetries or disturbances in the outer regions, but no clear signs of major mergers or tidal tails are evident. The galaxy has a relatively compact apparent size.
