The galaxy presents as an elliptical morphology, appearing largely smooth and rounded. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The galaxy's color profile suggests a relatively evolved stellar population, with a dominant yellowish-red hue in the core. There is a subtle blue-ish tint visible in the outer regions, indicating a small amount of on-going star formation, or potentially a population of younger, bluer stars. No spiral arms or bar structures are discernible. No signs of major disturbances due to mergers are apparent, though slight irregularities in the outer isophotes cannot be ruled out. Overall, the galaxy appears to be a relatively isolated and undisturbed system.
