The galaxy presents as a luminous, elliptical morphology with a bright, concentrated central bulge. The color profile suggests an older stellar population, appearing predominantly yellow to orange.  There is a slight indication of a possible tidal tail extending from the main galactic body, suggesting a past interaction or merger event.  The overall structure appears relatively smooth, without prominent spiral arms or distinct dust lanes.  The light distribution is generally symmetrical, with a gradual decrease in brightness from the core outwards. There is some faint and very distorted disc structure present. Based on the surrounding features, this galaxy is likely a significant mass and size relative to other galaxies in this field of view. 
