The galaxy presents a largely smooth morphology, with a dominant central bulge. It appears elliptical in shape, not showing any obvious spiral arm structure. Color gradients suggest a radial variation in stellar populations, transitioning from slightly redder hues in the center to somewhat bluer tones in the outer regions of the galaxy. This could be due to older stars concentrated in the center, with more recent star formation occurring in the outer regions. There is a minor disturbance in the smoothness of the galaxy that could be tidal debris. The galaxy doesn't look to be undergoing a major merger. The overall round shape is generally smooth and mostly round in appearance.