The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color appears predominantly yellow-orange, suggesting an older stellar population with a lower rate of star formation. No distinct spiral arm structures or significant dust lanes are apparent. There may be a faint tidal tail or plume present to the lower left side of the galaxy. There is a small indication that the galaxy is not perfectly round, but the ellipticity is not extreme. This galaxy appears to be relatively undisturbed, with no major signs of ongoing or recent merger events.
