The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The core exhibits a concentrated, luminous glow, with a gradual decrease in luminosity towards the outer regions. There is a subtle color gradient observed, with the central regions exhibiting a yellowish hue, transitioning to a redder tone in the outer areas. No distinct spiral arms or significant dust lanes are discernible within the visible structure. Based on the overall form and color profile, the stellar population is likely dominated by older stars. There is no indication of major merger events or significant tidal disturbances impacting the galaxy.
