The galaxy presents as a luminous, somewhat compact elliptical galaxy with a high degree of central concentration. It appears quite smooth, with minimal discernible substructure or spiral arms. The galaxy exhibits a predominantly yellowish hue in its central region, suggesting a relatively old stellar population. Fainter, reddish light is observed around the core, potentially indicating the presence of a population of cooler stars. There is no obvious distortion or interaction apparent in the immediate vicinity of the galaxy, which suggests the system is relaxed. The object's morphology is consistent with a high probability of being a smooth elliptical galaxy.
