The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core, likely indicating a high stellar density. The light profile decreases gradually from the core outwards, forming a diffuse halo. There is no significant evidence of spiral arms or a distinct disk structure in the image, rather it appears to be a spheroid galaxy. Faint irregular features are present in the galaxy which may point to minor tidal interactions. The color is generally consistent across the galaxy, appearing yellow-white, with some hints of green. This suggests the presence of intermediate to old stellar populations and a moderate amount of on-going star formation. The observed redshift indicates a substantial distance, and the physical size of the galaxy, while somewhat compact, is significant in terms of kiloparsecs. The galaxy appears relatively isolated, with no obvious nearby companions or other signs of major merging activity.
