The galaxy appears as a centrally concentrated object with a smooth, diffuse light distribution. Its shape is generally elliptical, exhibiting an elongation rather than a perfectly circular profile. There is no obvious presence of spiral arms or significant dust lanes. The color gradient transitions from a bluer, more vibrant hue at its core to a redder, more subdued tone in the outer regions, suggesting a possible difference in stellar populations or dust content between the central and peripheral areas. There are no signs of major mergers or tidal distortions, although minor disturbances cannot be ruled out. The galaxy is relatively compact, with its light source being located near the center of the object. 
