The galaxy appears as a largely smooth, centrally concentrated object. Its light profile is well-resolved and the galaxy exhibits a predominantly elliptical morphology. There are no distinct spiral arm structures visible. The color appears relatively uniform across the galaxy, showing a bias toward redder wavelengths, indicating an older stellar population and/or significant dust obscuration. There is little evidence of ongoing, vigorous star formation, rather a more quiescent, evolved system. The general structure suggests that it may be undergoing a period of relative calm. The galaxy is not undergoing a major merger, nor significant tidal disruption.
