The galaxy presents a somewhat elongated morphology, appearing as an intermediate shape between round and cigar-like. The central region exhibits a smooth, concentrated distribution of light, with a noticeable yellow-orange hue, potentially indicative of an older stellar population. There is evidence of some disturbed arms or features within the galactic disk or halo surrounding this center. In addition, some redder, compact regions are visible on either side of the central region, suggesting active star formation. These appear quite small and faint. The galaxy's overall structure does not exhibit signs of a major merger, although there may be minor disturbances present, causing the lumpy shape. The color gradient suggests ongoing, but perhaps declining, star formation activity within the galaxy.
