The galaxy presents as a largely smooth, elliptical-like structure. There is a concentrated central bulge, exhibiting a yellowish hue, likely indicative of an older stellar population. The surrounding halo appears more diffuse, with a bluer tint, which may suggest regions of ongoing, though perhaps modest, star formation. The overall morphology is quite regular, displaying a high degree of circularity. There is no obvious evidence of any major mergers or significant tidal disturbances within the immediate vicinity of the galaxy. Faint extended features are observed, but they are not prominent enough to disrupt the smooth overall appearance.
