The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. It exhibits an elliptical-like appearance, with a gradual decrease in surface brightness moving outwards from a bright, nearly spherical core. The color gradient suggests a population of older stars, appearing redder in the outer regions and yellow closer to the core. There is no significant evidence of spiral arms, a prominent disk, or active star formation regions within this image. There may be some minor disturbance within the galaxy, but it seems to be overall relatively undisturbed. Overall, the galaxy appears to be a mature, relatively massive system dominated by an older stellar population.
