The galaxy presents as a relatively smooth, elliptical form, appearing somewhat elongated. Its light profile indicates a concentrated central region with a gradual decrease in luminosity towards the outer edges. The galaxy exhibits a bluish hue, suggesting the presence of a population of relatively young, hot stars within its structure, although it is not dominated by them. There appears to be little to no evidence of spiral arms or significant dust lanes. The overall impression is of a galaxy in a relatively quiescent state, lacking any obvious signs of recent major mergers or intense star formation across the whole galaxy.
