The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a bright, concentrated luminosity suggestive of a prominent galactic bulge or active galactic nucleus. Proceeding outwards from the center, the light gradually diffuses into a more irregular shape with a smoother appearance. The overall color profile indicates a mix of stellar populations. The inner core is a golden hue that transitions into bluer tones towards the outer edges. These varying colors suggest active star formation regions within the galaxy and a distribution of older, redder stars elsewhere. There is a very slight hint of disk features present with very faint spiral arm features. There appears to be no major disturbances nor significant signs of ongoing merger activity.
