The galaxy presents as a lenticular or edge-on spiral type, with a noticeable central bulge. The bulge appears relatively smooth and concentrated, suggesting an older stellar population. A faint, extended disk is visible, though it is tilted nearly edge-on to our line of sight. The disk exhibits a blue hue. There is a slight indication of dust lane obscuration along the central plane of the galaxy, but the overall structure is relatively undisturbed, showing no signs of a major merger or significant tidal disruption. The overall apparent size is relatively small.
