The galaxy presents as a lenticular or early-type spiral galaxy, seen at a slight angle. The central bulge is prominent and exhibits a reddish-yellow hue, possibly indicative of an older stellar population with lower levels of star formation. Surrounding the bulge is a fainter disk component, which appears relatively smooth. There are hints of spiral arm structure, but they are not well-defined. The galaxy appears to be moderately massive. There might be very faint signs of minor disturbances, but it is difficult to ascertain merger activity.
