The galaxy presents a primarily smooth morphology. The central region exhibits a high concentration of luminosity, appearing as a bright, concentrated core. Surrounding this core is a more diffuse halo of light, extending outwards with an irregular shape. There is a slight asymmetry in the halo's light distribution. A faint disturbance to the right side of the galaxy could indicate minor gravitational interaction with a smaller nearby object or recent merger. The colours seem to be slightly offset within the inner core.
