The galaxy presents as a largely featureless, elliptical structure with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light appears to fade gradually towards the outer regions, which display a slightly bluer tinge. There is a faint suggestion of a disk, but no readily identifiable spiral arm structure. No prominent dust lanes or recent star formation regions are visible. The overall morphology indicates a relatively quiescent galaxy with a moderate mass and low star formation rate, with no significant indications of ongoing mergers or tidal disturbances. Its round shape also indicates a later stage of galactic evolution.
