The galaxy presents as a moderately luminous, relatively compact system with an elliptical morphology. The central region exhibits a strong concentration of light, indicative of a dense stellar population. This core transitions smoothly into a diffuse halo or envelope, characterized by fainter, more spatially extended emission. There is a subtle color gradient observed, with the central region appearing slightly redder than the outer regions. This may suggest a difference in stellar populations, with older, redder stars concentrated towards the center and a slightly younger, bluer population in the outskirts. Overall, the galaxy appears largely undisturbed, with no obvious signs of significant tidal interactions or recent mergers. There is a hint of what may be a very faint and diffuse disk extending from the central region.
