The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge with a gradual decline in luminosity towards its outer regions. There is an absence of prominent spiral arms or significant dust lanes, which supports a classification as an elliptical galaxy. The light distribution is fairly symmetrical, and the galaxy has a yellow-reddish hue, possibly indicating an older stellar population with a low rate of star formation. It shows a nearly round morphology. There are no obvious signs of tidal disturbances or interaction with other galaxies.
