This galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. It presents a concentrated central bulge, which gradually fades into the outer regions. The overall color index suggests a population of older stars, leaning towards the redder end of the spectrum. The galaxy exhibits a slight roundness and no visible signs of active merging or significant disturbances. The light distribution suggests a centrally concentrated mass distribution. Star formation activity appears to be quiescent or suppressed within this system.
