The galaxy presents as a relatively smooth, elliptical morphology. The central bulge is clearly defined and exhibits a bright, concentrated luminosity gradient indicating a high density of stars. A more diffuse halo surrounds the central bulge, with a gradual decrease in luminosity towards the outer regions. There is very little evidence of spiral arm structure or distinct features within the disk. The overall shape is close to round, with only a slight elongation. There is some indication of minor disruption on the left side of the halo, perhaps due to a minor tidal interaction or internal dynamic process. Based on the color gradient from the center outwards, we can infer the stellar population composition. The central regions appear more yellow/orange, suggesting a population of older, cooler stars, while the outer halo shows bluer regions, perhaps indicating some pockets of more recent star formation. 
