The galaxy presents as a moderately luminous, disk-shaped system. It exhibits a central bulge that appears nearly spherical and dominates the overall brightness of the galaxy. The bulge displays a yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation in that region. 

Surrounding the bulge, a faint disk is visible. The disk appears somewhat inclined to our line of sight. Its color is slightly bluer than the bulge, indicating the presence of younger, hotter stars, and possibly some ongoing star formation. The galaxy appears relatively smooth in structure, with no prominent spiral arms or dust lanes immediately apparent. However, there is a redder, possibly dusty region on the edge of the disk. There are no signs of major mergers or significant tidal disturbances.
