The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits high luminosity, appearing significantly brighter than the surrounding galactic structure. This suggests the presence of a substantial central bulge. The overall shape is approximately round, with no obvious spiral arms or significant disc structures visible. There's a subtle colour gradient observed, transitioning from a yellowish-white core to a slightly bluer hue in the outer regions. This may indicate a shift in stellar populations, with older stars dominating the central bulge and younger stars contributing to the outer regions. No signs of tidal disturbances, major mergers, or active galactic nuclei activity are readily apparent in the image. The galaxy appears relatively isolated and undisturbed.
