This galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a bright, yellowish-white hue, potentially indicative of a dense population of older stars. Moving outward, the color gradually shifts towards a redder tone, which could suggest a lower density of younger, bluer stars in the outer regions. The overall form appears relatively undisturbed, showing no clear signs of major mergers or significant tidal interactions, although subtle irregularities in the outer halo cannot be ruled out completely at this resolution. The galaxy seems to be on the larger side, with a noticeable extended halo. There is a distinct absence of prominent spiral arms or significant dust lanes. The galaxy's morphology suggests it is an older system, possibly undergoing relatively low levels of star formation.
