The galaxy presents a predominantly smooth morphology, exhibiting a well-defined central bulge. The overall shape appears largely elliptical, with a high degree of roundness and only minimal deviation toward an elongated or cigar-like form. There is an absence of readily apparent spiral arm structures or significant dust lane features. The galaxy appears undisturbed, lacking any obvious signs of ongoing major mergers or tidal interactions. Faint, diffuse extensions surrounding the main body may indicate the presence of a stellar halo, though this feature is subtle. Color gradients suggest a relatively evolved stellar population, particularly within the bulge. There is some blue light showing areas of star formation.