The galaxy presents as a single, relatively smooth structure with a centrally concentrated light profile. It exhibits an elliptical morphology, appearing largely spheroidal in shape. There is a slight elongation visible, however the galaxy is mostly round. The color gradient shows a dominant yellowish-orange hue toward the center, suggesting an older stellar population. The outer regions of the galaxy fade gradually into the background, with faint hints of greenish-blue, potentially indicating some low-level star formation activity in the outer disk. There is no discernible evidence of spiral arms or prominent dust lanes and the galaxy is not undergoing a major merger. The overall appearance is consistent with a mature galaxy.
