The galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth morphology with a high degree of central concentration. The core is bright and appears to be nearly spheroidal. Extending outward from the core, the galaxy demonstrates a diffuse halo. There's a subtle color gradient, with the central bulge appearing slightly yellower than the outer regions, suggestive of an older stellar population concentrated in the center. The overall structure is relatively undisturbed, with no signs of significant tidal interactions or major mergers. A very slight asymmetry in the outer halo could indicate a past minor merger or accretion event, but further investigation is required to confirm this. 
