The galaxy presents a relatively smooth morphology, with a bright central bulge that gradually fades into the outer regions. It appears to be a disk galaxy viewed at a slight angle. A subtle disk structure is observed around the central bulge, indicating the possible presence of spiral arms although the resolution limits a firm conclusion. The galaxy exhibits a yellowish-white color gradient, with the central bulge appearing more yellow, suggesting an older stellar population. Star formation appears to be somewhat active, but is not strong, particularly in the nuclear region. Fainter blue hues in the outer disk suggests ongoing but limited star formation. There are no obvious signs of major mergers or significant tidal disturbances. Overall, the galaxy appears to be in a relatively quiescent state, and is mostly unperturbed.
