The galaxy presents a somewhat rounded morphology, appearing largely smooth with a moderate concentration of light towards its center. There is a hint of asymmetry, particularly in the upper region of the galaxy, where a diffuse extension or possible tidal feature is observed. The color gradient suggests the presence of ongoing or recent star formation activity, with bluer hues concentrated in the central and upper regions, potentially indicative of younger stellar populations. The galaxy shows a yellowish-red component as well, which is distributed more diffusely, likely representing older stellar populations or dust. This galaxy may be undergoing a minor interaction or merger event based on the morphological disturbances, although a significant portion of the galaxy remains relatively undisturbed. The light appears to be relatively dim.
