The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution. It possesses a central bulge that appears to be largely composed of older stellar populations, judging by its yellowish-red hue. Fainter, bluer regions can be seen in the outer disk, hinting at ongoing or recent star formation. The overall structure appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. It is elongated, with a length that looks to be approximately twice its width. There is minimal indication of spiral arm structure or prominent dust lanes.
