The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish hue, suggestive of an older stellar population. There appears to be little to no evidence of prominent spiral arms or significant dust lanes. The galaxy is largely spheroidal, with an observed axis ratio close to 1, indicating a nearly circular projected shape. There are no obvious signs of major ongoing mergers or tidal disturbances. Faint features suggesting minor interactions with nearby companions cannot be ruled out based on the available image resolution, though the overall morphology appears relatively undisturbed. It is a massive galaxy with a low rate of star formation.
