The galaxy presents as a relatively smooth, elliptical-like object. It has a concentrated central bulge that emits strongly in the red and green portions of the spectrum, giving it an overall yellowish-orange hue. The galaxy appears mostly undisturbed, with no obvious signs of ongoing major mergers or significant tidal features. A faint, diffuse halo extends outward from the central region, exhibiting a bluer color compared to the core, potentially indicating a population of younger stars within the outskirts. The shape of the galaxy is somewhat rounded, though not perfectly circular, with a slight elongation in one direction. The overall structure indicates a system dominated by an older stellar population, though some degree of star formation may be present in the outer regions.
