The galaxy presents as a relatively smooth, elliptical-like structure with an approximate effective radius of 6.4 kpc. There is little discernible fine structure; no spiral arms, bar features, or prominent dust lanes are visible. The color profile suggests a more pronounced concentration of older stellar populations in the central regions, indicated by the yellowish hue, while the outer regions exhibit a slightly bluer tint, possibly reflecting more recent, albeit limited, star formation. The overall morphology appears to be relatively undisturbed, with no obvious signs of recent major mergers or significant tidal interactions, though some minor disturbances cannot be ruled out. The galaxy exhibits an intermediate axial ratio, neither perfectly spherical nor highly elongated.
