This galaxy presents a primarily smooth, elliptical morphology. Its core exhibits a concentrated, yellowish hue, suggesting an older stellar population. The central bulge appears significant, indicating a substantial mass concentration. 

Faint, diffuse extensions are visible to one side, potentially indicative of tidal interactions or minor disturbances. These features display a slightly bluer color, suggesting the presence of younger stars, or perhaps evidence of active star formation regions. The galaxy appears to be in a relatively isolated environment, and there is no clear evidence of a major ongoing merger. However, a possible tidal feature suggests a past interaction. The primary light distribution has an ovoid shape, with an intermediate axial ratio.
