The galaxy presents a generally elliptical morphology, though with some observed asymmetry. The core region exhibits a concentrated, bright luminosity, appearing yellowish-orange in color. This suggests a population of older stars dominating the nuclear region. Moving outwards from the core, the light diffuses, showing a smoother distribution. There is evidence of a faint extension to one side of the main body. This extension seems less bright and bluer in color, hinting at ongoing, though possibly subdued, star formation in this outer region. The overall structure appears relatively smooth, with no obvious spiral arm features. The galaxy presents a non-negligible redshift, indicative of its considerable distance.
