The galaxy appears to be an elliptical or lenticular type. It has a generally smooth, concentrated morphology with a noticeable central bulge. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy exhibits a radial color gradient, with a bluer core and redder outer regions. This color gradient suggests a mixture of stellar populations, with younger, hotter stars concentrated in the central region, and older, cooler stars dominating the outer regions. The galaxy exhibits very slight disturbances which may indicate a minor merger.
