The galaxy presents as a predominantly smooth, elliptical morphology. There is a slight elongation to its shape, suggesting a possible deviation from perfect sphericity. The galaxy exhibits a color gradient, appearing slightly bluer in the central region and becoming redder towards its periphery. There are no obvious signs of spiral arms or significant dust lanes. No major disturbances are visible, implying it is not currently undergoing a major merger. The galaxy appears relatively isolated, with no nearby interacting companions immediately evident in the image.
