The galaxy presents a primarily smooth, elliptical morphology, viewed approximately edge-on. It exhibits a pronounced central bulge that dominates the overall light profile. A flattened disk component is visible, oriented perpendicular to the line of sight. The disk appears to be relatively featureless, lacking prominent spiral arms or distinct dust lanes. The galaxy's color gradient indicates a potentially older stellar population, particularly within the bulge, based on its relatively redder hue. Some degree of disturbance is seen, likely not a recent major merger, but perhaps signs of a minor gravitational interaction. The general shape might indicate some past merger. Overall, the galaxy shows some structural irregularity and possibly some tidal features, even if they are faint, in its outer halo, suggesting a history of gravitational interactions.