The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, showing a round form with minimal deviation from circularity. There is no distinct spiral arm structure visible. Faint hints of a disturbed morphology are present; possibly either an interacting companion galaxy or an internal disturbance within the galaxy itself. The galaxy displays a broad color profile ranging from blue, green, and red. The brighter regions suggest an evolved stellar population. Overall, this galaxy presents as a relatively massive system with signs of a possible, past merger.
