The galaxy appears to be a relatively compact object with a smooth, elliptical morphology. The light is centrally concentrated with a bright, nearly unresolved core, indicative of a substantial bulge component. The galaxy's overall shape exhibits a slight elongation. There is no discernible disk structure or spiral arms, nor is there any evidence of recent major merger activity or significant tidal disturbances in the immediate vicinity. The galaxy presents a relatively featureless appearance. The light profile transitions smoothly from the bright core outwards, with a gradual decrease in surface brightness. The color appears roughly uniform across the galaxy, with a subtle shift toward redder hues in the outer regions, suggesting an older stellar population dominating the halo.
