The galaxy presents a predominantly smooth, elliptical morphology. There is a slight elongation, but it largely appears spheroidal. The color profile exhibits a gradient, with a central concentration of yellow-red hues that gradually fades to a bluer periphery. This color distribution is indicative of an older stellar population dominating the central region, potentially with ongoing, lower-level star formation in the outer regions. There appears to be significant gravitational interaction occurring; possibly a merger. It is most likely in the late stages of this event, due to its lack of distinguishable disturbances.
