The galaxy presents as an elliptical, relatively smooth structure with a slightly elongated morphology. The galaxy exhibits a color gradient, appearing more yellow or golden in the central regions, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes within the galaxy. A small blue region appears to be present on one side of the galaxy, possibly indicating a region of ongoing star formation. The overall appearance is consistent with an early-type galaxy that is relatively quiescent in terms of star formation activity but still possesses a notable stellar mass. There are no obvious signs of a recent or ongoing major merger event, though there could be minor disturbances in the overall shape.