The galaxy presents a morphology that is neither purely elliptical nor a well-defined spiral. There is evidence of a central bulge component, with an intermediate size. Disk features are present, but the galaxy does not exhibit a clear spiral arm structure and is mostly smooth.

Based on the slight asymmetry and other disturbances, there is evidence that this galaxy is undergoing or has undergone a merger with another galaxy, or experienced another significant gravitational disturbance, which can be either a minor disturbance, major disturbance, or a merger.
