The galaxy presents a generally smooth appearance with a slightly elliptical morphology. It exhibits a concentrated central bulge which is yellowish-white in color.  The outer regions of the galaxy are more diffuse and appear slightly flattened. There's a subtle suggestion of a faint, extended disk surrounding the central bulge, however no obvious spiral arm structures are present. The overall color profile suggests a population of older stars. No signs of a major ongoing merger or significant tidal disturbances are clearly visible; however, there is some potential evidence of minor irregularities in the outer regions that could suggest previous interactions. The galaxy appears relatively isolated.
