The galaxy presents as a centrally concentrated, yellowish-white elliptical or lenticular system. The central region exhibits a smooth, diffuse appearance, indicating a relatively old stellar population. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology appears to be largely spheroidal, with a gradual decrease in luminosity from the core outwards. There is a slight elongation observed. Given the color and smooth texture, star formation activity appears minimal. The lack of any tidal tails or distortions suggests that the galaxy is not currently undergoing a major merger event.
