The galaxy appears to be a relatively smooth and featureless elliptical galaxy, with a slightly elongated shape that is close to round. It exhibits a central bulge that is slightly brighter and denser than the surrounding regions. The galaxy has a dominant blue hue, suggesting the presence of a population of younger, hotter stars. There is little evidence of spiral arms or significant dust lanes. The overall morphology appears relatively undisturbed, with no clear indications of major recent merger events, although some minor disturbances cannot be ruled out. The estimated size of the galaxy suggests it is relatively small. Low levels of star formation are ongoing.