The galaxy presents a smooth, elliptical morphology, with a centrally concentrated luminosity profile. The object exhibits a predominantly round shape. There is a notable absence of any prominent disk-like structure or spiral arms. The core region displays a bright, yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy transition to a fainter, slightly reddish color. There is no evidence of significant dust lanes, tidal tails, or merging features. Based on the smooth and centrally concentrated light distribution, this galaxy is classified as an elliptical galaxy. The color gradients suggest a potential variation in stellar populations, with older, redder stars dominating the outskirts and a younger, more metal-rich population concentrated in the central regions.
