The galaxy exhibits a generally elliptical morphology, though not perfectly circular. There is a smooth, gradual transition in brightness from the core outwards, suggesting a relatively evolved stellar population and a Sersic index implying a possible disk-like component within the galaxy's structure. The galaxy's color profile indicates a mix of stellar populations, with a slightly bluer hue in the outer regions, possibly indicating recent or ongoing star formation activity at a low rate. The galaxy exhibits a clear bulge, with higher concentration of older stars. There are no strong indications of active galactic nuclei activity or prominent dust lanes based on the color and smooth texture of the galaxy. No spiral arm structure is visible, instead there is a rather uniform light distribution.
