The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated core that gradually fades into a diffuse halo. The core appears slightly reddish, possibly indicating an older stellar population or significant dust obscuration within that region. The outer halo shows a subtle bluish tinge, which might suggest the presence of a younger, bluer stellar population. There is no readily apparent spiral structure or disk component; the light distribution is largely spheroidal. No significant tidal features or signs of ongoing major mergers are observed in the immediate vicinity of the galaxy, though there may be a slight asymmetry in the outer regions, potentially indicative of a minor interaction.
