The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The core region exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. A subtle color gradient is observable moving outwards from the center, transitioning to a slightly bluer hue within the galaxy's intermediate regions, possibly indicative of a low level of ongoing star formation. The galaxy appears to be fairly isolated with little to no signs of tidal disturbance or interaction with other galaxies. The galaxy is fairly large with an estimated size on the order of 3.7 kiloparsecs. Overall, it appears to be a massive galaxy that is approaching a state of quiescence in its star forming capabilities.
