The galaxy presents a largely smooth morphology, exhibiting a concentrated central bulge that dominates its overall structure. The core region appears yellowish, potentially indicating an older stellar population. Surrounding the core is a fainter, more diffuse halo of light that extends outwards, exhibiting a slight elongation. There are faint traces of a disk-like structure, but these are not well-defined. Overall, the galaxy appears relatively undisturbed, without any obvious signs of ongoing major mergers or tidal interactions. There may be some minor disturbances.
