The galaxy presents a generally smooth, elliptical morphology. Its core region exhibits a concentrated, bright luminosity, appearing yellowish-white in color. Moving outward from the core, the galaxy's light gradually diffuses, transitioning to a slightly bluer hue in the outer regions, suggesting a possible population of younger stars. The overall shape approximates a slightly elongated spheroid, showing a tendency towards an 'in between' level of roundness, with minimal evidence of a distinct disk structure or spiral arms. There is a subtle asymmetry present in the outer halo. The galaxy appears to be relatively isolated, without any obvious signs of major mergers or significant tidal disturbances, though it appears to display a minor disturbance.
