The galaxy presents as a fairly smooth and elliptical structure. It appears highly rounded. The central bulge exhibits a concentrated brightness, with a yellowish-white hue, suggesting a population of older stars. There is little to no visible disk component or spiral arm structure, and no apparent dust lanes. The outskirts of the galaxy gradually fade into the background sky, indicating a lack of sharp boundaries. It does not appear to be undergoing any major mergers or tidal interactions, although there may be minor disturbances present. The galaxy's color gradient suggests a relatively uniform stellar population throughout its structure, with a consistent progression from the bright core outwards.
