The galaxy appears to be a relatively smooth, elliptical-like structure. The core exhibits a concentrated, yellowish hue, suggesting an older stellar population likely dominating the central region. Moving outward from the core, the galaxy gradually diffuses, transitioning into a bluer halo. This halo appears to be composed of a more dispersed distribution of stars and potentially gas. There is a subtle hint of disk like structure and the galaxy is not perfectly round, showing a slight elongation. Overall, there are no significant signs of major disturbances or ongoing mergers that would drastically alter the overall structure of the galaxy. The observed color gradient suggests a gradient in stellar populations, with older stars concentrated in the core and a relatively younger, bluer population present in the outer regions.
