The galaxy presents as a largely elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. The core region displays a notably bright and somewhat reddish hue, gradually transitioning to a greenish-yellow color in the outer regions. The structure appears moderately rounded. There are no visually apparent signs of spiral arms, bars, or significant dust lanes. Subtle irregularities in the outer halo suggest the possibility of minor gravitational interactions or past mergers. The overall impression is that of a galaxy that is relatively evolved, exhibiting moderate to high rates of star formation.
