The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. The galaxy has a prominent central bulge that fades gradually into the outer regions without any sharp edges or spiral arm structures. The galaxy exhibits a color gradient, transitioning from a redder hue in the central region to slightly bluer tones in the periphery. There are no apparent dust lanes or significant signs of ongoing star formation within the galaxy. The overall shape suggests a relaxed, spheroidal structure with a possible slight ellipticity, and does not appear to be undergoing any major merger events or gravitational disturbances.
