The galaxy presents a relatively smooth, elliptical morphology. A concentrated central bulge is observed, exhibiting a yellowish-white hue, suggestive of an older stellar population. Extending outwards from the bulge is a more diffuse, bluish halo. This color indicates the presence of younger, hotter stars, although their distribution appears relatively homogenous without prominent spiral arm structures. The overall shape deviates slightly from perfectly circular, exhibiting a mild elongation that may indicate a triaxial structure or potential interaction, though no clear tidal features are visually apparent.
