The galaxy presents a generally smooth and elongated morphology, appearing as a disk that is viewed at an oblique angle from our vantage point. The central region exhibits a high degree of luminosity, appearing nearly spheroidal and gradually decreasing in brightness towards the edges. There's a subtle blue hue particularly noticeable towards the extremities, suggestive of younger stellar populations and potentially ongoing star formation activity. The overall structure reveals characteristics of an intermediate disk galaxy without any obvious signs of major mergers. Faint tidal features or minor disturbances can not be ruled out.
