The galaxy appears to be an elliptical galaxy, elongated in shape. It exhibits a smooth, featureless morphology, lacking prominent spiral arms or a distinct disk structure. The light is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. The color appears to be redder than average, suggesting a population of older stars with lower star formation activity. The galaxy does not show any signs of a major ongoing merger, but possible minor disturbances could be occurring.
