The galaxy presents a generally smooth morphology, appearing elliptical in shape, with a slight elongation. Its core is bright and concentrated, indicating a significant concentration of stars or potentially an active galactic nucleus. The light distribution fades gradually from the center outwards, suggesting a lack of distinct spiral arms or prominent features. The overall color appears to be redder, possibly indicative of an older stellar population or significant dust obscuration. There are no obvious signs of recent mergers or major disturbances in its structure, although a subtle asymmetry might be present.
