The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a dominant central bulge with a concentrated luminous core. The light profile diminishes gradually from the center outwards, displaying no prominent spiral arm features or distinct dust lanes. The color is a yellow-orange hue, indicative of a population of older stars. There might be a faint and subtle disk component, as suggested by a slight elongation in its shape, but the overall morphology is that of a spheroid. There is no visual evidence of strong tidal interactions or major disturbances in the immediate vicinity, although there could be minor disturbances within the galaxy itself.
