The galaxy presents as a relatively smooth, centrally concentrated object. It displays a somewhat elliptical morphology, appearing nearly round but possibly with a slight elongation. Its color profile shows a strong central concentration of light, with the core exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions display a gradual color gradient, with some faint bluish and greenish tones possibly suggesting areas of more recent star formation. There is some indication of minor disturbances in the morphology, possibly indicating a past merger event or tidal interaction, but overall the galaxy is not heavily distorted. There are no readily apparent spiral arms or a pronounced disk structure, and the galaxy lacks any evidence of intense, ongoing star formation.
