The galaxy appears to be a spiral galaxy, though perhaps more closely resembling a lenticular (S0) type. The central bulge exhibits a smooth, concentrated luminosity profile. The disk surrounding the bulge is relatively smooth, with only a few faint, broad spiral arm-like structures distinguishable. These features are relatively unstructured and diffuse, suggesting that the galaxy is evolving slowly. The overall shape is moderately elliptical with a intermediate roundness. There is minor disturbances in the galaxy, suggesting it could be undergoing a minor merger event. Its mass indicates it is a moderate sized galaxy, but given that the star formation rate is moderately low, the galaxy could eventually become an elliptical galaxy.
