The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. Its color profile is predominantly yellow, suggesting a stellar population dominated by older, redder stars, which could be indicative of reduced recent star formation. The overall rounded shape indicates a low degree of internal rotation and a lack of prominent spiral arm structures. There are no obvious signs of major mergers or significant tidal disturbances. Minor disturbances may be present. The galaxy appears to be relatively isolated with no immediately apparent companion galaxies.