The galaxy exhibits a smooth, elliptical morphology. It displays a gradual increase in surface brightness towards the center, indicating a centrally concentrated stellar population. The galaxy's shape is somewhat elongated, though not strongly cigar-shaped, appearing more intermediate in roundness. There is no obvious evidence of spiral arms, dust lanes, or significant star-forming regions in this image. The overall color suggests a relatively old stellar population. There is no strong evidence of interaction or merging with other galaxies. The overall structure appears relatively undisturbed.
