The galaxy presents as a luminous, centrally condensed object with a dominant smooth component. The overall morphology appears approximately circular. The color profile suggests a higher concentration of younger stellar populations, indicated by a bluer hue, particularly in the central region. There may be evidence of tidal disturbances or minor interactions, though the main body retains a relatively undisturbed morphology. Areas of increased brightness are visible. It does not present as a grand spiral or barred spiral structure. A fraction of light exhibits a redder colour than most of the galaxy.
