The galaxy presents a generally smooth morphology, appearing elliptical in shape. There is a subtle central concentration of light, with luminosity gradually decreasing outwards from the core. The galaxy appears to be dominated by an older stellar population, which makes it appear generally redder. No spiral arms or distinct disk-like features are readily apparent. The structure suggests minimal ongoing star formation. There is no evidence of major disturbances or interactions with other galaxies. The galaxy exhibits a moderate redshift, indicating a considerable distance.
