The galaxy presents as a luminous, centrally concentrated object, exhibiting a morphology that is predominantly smooth in appearance. The light distribution suggests a spheroidal shape, though not perfectly circular; there is a slight elongation apparent. The galaxy's core region demonstrates the highest surface brightness, with a gradual decrease in luminosity extending outwards. There is faint structure that could be described as a mild disturbance, possibly indicative of a minor interaction or internal dynamic process. A redder hue seems to be present relative to the rest of the light, meaning older stars. The estimated size appears to be substantial, suggesting a relatively massive system. Overall, the features observed are consistent with a massive galaxy that has largely completed its star formation.
