The galaxy presents as a spiral structure, with a clearly discernible disk component. The disk exhibits a notable feature, likely a bar, which appears to bisect the galaxy's central region. Spiral arms are visible, extending outwards from the bar. The arms appear loosely wound, and are not very well defined. A central bulge is evident, representing a significant fraction of the galaxy's overall light. There are no obvious signs of major mergers or tidal disturbances. The galaxy appears to be at a significant distance, as indicated by its small angular size.
