The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology leans towards elliptical. There is minimal discernible disk structure or spiral arms visible. The light profile exhibits a gradual decrease in intensity from the center outwards. Color gradients suggest a central concentration of older stars and a possible presence of younger, bluer stars in the outer regions, although these regions are subdued. Evidence of any major mergers or significant disturbances is lacking. The galaxy appears largely undisturbed and potentially evolved.
