The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in surface brightness outward. The overall color is indicative of an older stellar population, with a subtle reddish hue dominating. There appears to be little to no evidence of spiral arms or prominent dust lanes. I observe a slight deviation from perfect circularity, leaning towards an 'in-between' elliptical shape with a hint of elongation. There is no visible sign of any major disturbance or ongoing merger, although there are some indications of minor irregularities that could be interpreted as a very slight disturbance. The galaxy possesses a moderately high mass, based on its brightness and inferred stellar population. Star formation appears to be quite low within the galaxy.

