The galaxy presents as a roughly elliptical, somewhat compact object. The light distribution appears relatively smooth, though there is some indication of underlying structure. There is a region which seems to have brighter blue-shifted light. It may indicate a region of active star formation or a knot of younger, hotter stars. Given the overall morphology and the presence of some smooth features, it is likely that the galaxy is a disk galaxy which is undergoing some kind of disturbance. There is also a suggestion of a possible tidal tail on one side of the galaxy.
