The galaxy presents as a somewhat diffuse, elliptical-like structure with a bright, concentrated central bulge. There is a subtle color gradient visible, transitioning from a more yellow/orange hue in the central region to a slightly bluer tint towards the outer edges of the visible disk. This could potentially indicate the presence of younger stellar populations in the outer regions compared to the older stars in the center. The galaxy exhibits a general smoothness with a lack of prominent spiral arms or distinct features. It seems relatively undisturbed, showing no strong signs of ongoing or recent major merger events, with only a few signs of minor disturbances. The light distribution appears even and consistent, with the bulk of the galactic mass concentrated in the core, and a gradual decrease in luminosity as one moves outward, though some clumping could be seen in the galactic halo. Based on the morphology and color distribution, I hypothesize this galaxy is a relatively massive system with a moderate star formation rate.
