The galaxy presents as a moderately bright, elliptical structure with a noticeable central bulge. The light distribution indicates a fairly smooth morphology with a distinct core.  The outer regions exhibit a subtle disklike structure, though it appears somewhat disturbed or irregular with possible faint tidal features. The main body of the galaxy displays a predominantly bluish-white hue, with tinges of green and red in the outer areas. These hints suggest a complex blend of stellar populations, gas and dust, and a possible merger event.  The galaxy lacks prominent spiral arms.  Its overall appearance implies ongoing activity, potentially triggered by interactions or accretion events.
