The galaxy presents as a centrally concentrated, relatively smooth object with a largely elliptical morphology. The core appears bright and concentrated, indicating a significant stellar population density. A gradual decrease in luminosity is observed from the center outward. The galaxy exhibits a yellowish hue, suggesting a population of older stars dominating its stellar content. The morphology indicates a likely evolved system with little to no readily apparent spiral arm structure or ongoing significant star formation, although very faint reddish regions may indicate some star formation. Overall, the object seems to be an early-type galaxy. The galaxy does not appear to be undergoing any major merger events or tidal disturbances, showing no signs of asymmetry in its light distribution.
