The galaxy presents as a spiral type, characterized by prominent spiral arms emanating from a central region. The arms appear relatively well-defined and exhibit a moderate degree of winding. A significant central bulge is noticeable, although it does not appear to dominate the overall structure of the galaxy. The presence of a bar structure is strongly suspected, bisecting the central bulge. The arms contain areas of bluer light, perhaps indicating regions of active star formation. There is no evidence of major mergers or significant tidal disturbance in the immediate vicinity of the galaxy, however a minor disturbance seems possible. The galaxy is not observed edge-on; it is presented at a more face-on orientation.
