The galaxy appears to be a relatively smooth, elliptical-like structure. There is a bright, concentrated central bulge with a distinct yellowish hue. A more diffuse halo surrounds the central region, fading gradually into the background. No distinct spiral arms or prominent dust lanes are visible. The galaxy exhibits an overall round shape with a slight elongation. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. The galaxy's color suggests a population of older stars, potentially indicating relatively low star formation activity. Faint hints of a redder outer halo may suggest a subtle color gradient.
