The galaxy presents as a smooth, elliptical object, elongated in shape. It exhibits a strong central bulge, characterized by a bright, concentrated luminosity suggestive of a high density of stars. Progressing outward from the center, the galaxy displays a gradual decline in surface brightness, with the outer regions appearing more diffuse. The color profile transitions from a yellowish-white core to a more reddish hue towards the periphery, potentially indicative of an older stellar population in the outer regions. There is no evidence of spiral arms or prominent dust lanes within the observable structure. The overall morphology suggests a relatively evolved system, likely of considerable mass. There are no obvious signs of ongoing major merger activity, though minor disturbances cannot be ruled out based solely on the image.
