The galaxy appears as a centrally concentrated object, exhibiting a largely smooth, spheroidal morphology. It lacks any easily discernible spiral arm structures or a prominent disk. The galaxy's light profile suggests a relatively homogenous distribution of stars, without substantial variations in color across its extent. The central region appears slightly brighter, suggesting a concentration of older stellar populations, or potentially an active galactic nucleus, though this cannot be confirmed from the available imagery alone. There might be evidence of a minor disturbance to the system, but the galaxy looks largely undisturbed. The round shape confirms it is not a spiral galaxy or disk galaxy and the lack of merger or tidal activity suggests it is well settled. Based on the red color, it is likely the galaxy is made of up of older stars, which means it could be a sizable elliptical galaxy.
