The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a moderately elongated shape, appearing cigar-shaped rather than perfectly spherical. A color gradient is observed, with a central concentration of yellowish light, potentially indicating a population of older stars. The outer regions appear fainter with slightly bluer hues, suggestive of a population of younger stars with ongoing star formation. There is no apparent spiral arm structure or prominent dust lanes visible. Overall, the galaxy's structure indicates a system undergoing moderate star formation with a substantial mass. There are hints of minor gravitational disturbances in the outer edges, but they do not appear to be major disruptions.
