The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. The color gradient suggests a stellar population that is likely a mixture of ages. There is evidence of a possible disturbance in its morphology as there are indications of some irregularity in the outer edges and a tail-like extension is seen at the bottom, possibly an interaction with a nearby galaxy. Overall it is not a perfectly spherical shape, and is slightly elongated. It does not exhibit a dominant disk structure, rather it appears to be a bulge-dominated system.
