The galaxy presents as a relatively small disk galaxy, viewed at an inclined angle. It exhibits a centrally concentrated bulge and a faint, diffuse disk. The light distribution indicates that the disk might be composed of an older stellar population, with the presence of neutral Hydrogen. There is a faint spiral arm structure, primarily on one side of the galaxy. The disk appears relatively smooth, suggesting the galaxy is likely undisturbed. The red-shift measurement puts the galaxy at a distance of about 89.8 Mpc and is in the zone of avoidance.
