The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated, circular morphology, with a noticeable radial color gradient. The central region presents a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the center, the color shifts towards a slightly redder tone, though the overall color profile remains relatively uniform. There is no discernible evidence of spiral arms, bars, or significant dust lanes within the visible structure. The galaxy lacks any obvious signs of ongoing major mergers or tidal disturbances, showing a fairly relaxed and symmetrical structure. Given the color and lack of features, star formation is likely low. The overall light profile suggests a de Vaucouleurs profile, consistent with an elliptical galaxy.
