The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a lack of distinct spiral arm structures or prominent dust lanes visible. The light distribution appears relatively uniform, with a gradual decrease in intensity from the center outwards. The galaxy appears relatively undisturbed with no signs of a major merger or tidal features. The roundness of the galaxy suggests a classification towards the E0-E3 range on the Hubble sequence. The galaxy exhibits a luminosity characteristic of a massive system. The overall color profile indicates a moderate level of ongoing star formation.
