The galaxy presents a generally smooth, elliptical morphology with minimal discernible substructure in this observation. The galaxy exhibits a concentrated central bulge that appears nearly spherical in projection. There is a gradual decrease in luminosity from the core outwards. Its color profile suggests an older stellar population, with a redder hue dominating the core region that transitions towards a slightly bluer tint on the periphery, consistent with ongoing, albeit limited, star formation in the outer regions. There is no evidence of spiral arms or a prominent disk component. No significant tidal features or signs of a recent major merger are apparent, though minor disturbances cannot be entirely ruled out.