The galaxy presents as a generally smooth, rounded object, visually consistent with an elliptical morphology. It displays a dominant, concentrated central bulge, exhibiting a yellow-orange hue, suggestive of an older stellar population. The absence of prominent spiral arms or significant dust lanes indicates a lack of active star formation. There is a slight asymmetry visible; a very subtle extension or tidal feature might be present on the periphery, potentially indicative of a past interaction or minor disturbance. Overall, the galaxy appears relatively isolated and well-defined.
