The galaxy presents as a spiral galaxy, inclined significantly to our line of sight, approaching an edge-on orientation. Prominent spiral arms are observed, though their detailed structure is somewhat obscured by the viewing angle. The bulge is moderate in size. A bar structure appears to exist along the major axis of the galaxy, though it is not particularly strong.

The galaxy exhibits a color gradient, with the central bulge displaying a yellowish hue, possibly indicating an older stellar population. The outer regions of the disk display a bluer tint, suggesting the presence of younger, hotter stars and ongoing star formation. There are no obvious signs of any major merger events or significant tidal disturbances in the immediate vicinity of the galaxy.
