The galaxy presents a generally smooth and rounded morphology. The light is concentrated in what appears to be a relatively compact central region, with a gradual decrease in brightness outwards. There is a slight elongation, but overall, the galaxy does not show strong indications of a disk-like structure. The color appears to be reddish, suggesting an older stellar population or significant dust obscuration. There is no obvious presence of spiral arms or active star-forming regions, based on the image. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger. A slight asymmetry in the light distribution might indicate a minor interaction, but the galaxy appears primarily relaxed and evolved.