The galaxy presents as a largely elliptical structure with a smooth, centralized concentration of light that diminishes gradually towards its outer edges. It exhibits a dominant yellowish hue at its core, suggestive of an older stellar population. Fainter, bluer tints are subtly apparent in the surrounding halo, hinting at the possibility of ongoing or recent star formation activity, albeit at a comparatively low rate. There is a slight asymmetry in the overall shape, potentially indicating a minor gravitational disturbance or interaction with a smaller, nearby companion galaxy. A faint, diffused halo envelops the primary structure.
