The galaxy appears as a generally smooth, elliptical-like structure. It exhibits a concentrated central region with a yellowish hue, potentially indicating an older stellar population. There is no clear evidence of distinct spiral arms or a prominent disk. The galaxy appears quite round in shape. Faint, diffuse extensions surround the central area, suggesting a gradual decline in stellar density outward. There is no evidence of any major mergers or interactions and only very subtle signs of disturbances.
