The galaxy appears as a singular, relatively smooth object with a concentrated center. The galaxy exhibits an elliptical morphology, showing no discernible spiral arm structure or distinct disk features in this image. The color profile suggests a dominant population of older stars, indicated by a yellow-red hue, although there is also blue light present. Based on this light, there is some ongoing star formation. There is no clear evidence of a major ongoing merger, tidal tails, or significant morphological disturbances. The galaxy is relatively compact in size.
