The galaxy presents a generally smooth morphology, suggesting an elliptical classification. It exhibits a concentrated, relatively symmetrical light profile with a gradual decline in brightness from the center outwards. The overall color is yellowish-orange. This hue could imply a relatively older stellar population dominating the galaxy's light output. No distinct spiral arm structures or prominent dust lanes are discernible in the image. The galaxy appears nearly spherical in shape, with a hint of possible elongation along one axis. There is no evidence of tidal tails or other significant disturbances, indicating it is likely not undergoing a major merger. Faint mottling is visible within the galaxy's halo, potentially indicating unresolved star clusters or minor structural features. Based on its apparent size and redshift, the galaxy appears to be a moderate-sized system. Star formation is likely suppressed or nearly absent.
