The galaxy appears as a relatively smooth, elliptical-like structure with a bright central region that decreases in intensity outwards. The object exhibits a yellow-reddish hue, indicative of an older stellar population. There is no strong evidence of spiral arms or prominent dust lanes visible in the image. There may be some faint features around the central area, which would suggest that there are no recent mergers or major disturbances. The smooth light profile suggests an evolved system with ongoing, but likely low, levels of star formation.
