The galaxy presents a primarily smooth, elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, yellowish-white coloration, suggestive of an older stellar population. Moving outward from the core, the intensity of light decreases, and the color transitions slightly towards a redder hue, possibly indicating the presence of evolved stars and/or dust extinction. The overall shape is largely spheroidal, with a slight elongation that could be due to intrinsic structure or projection effects. There is some subtle asymmetry noticeable in the outskirts, which may suggest minor gravitational interactions or past merger events. No distinct spiral arms or prominent dust lanes are discernible. There appears to be a slight reddish point-like source near the core, but whether it is associated with the galaxy or is a foreground/background object cannot be determined from this single image. Considering the color indices, the galaxy appears to host a relatively low amount of on-going star formation. The estimated size suggests this is a relatively large galaxy.
