The galaxy presents as a highly inclined disk galaxy, viewed nearly edge-on. A central bulge is prominent and exhibits a yellowish-orange hue, indicating an older stellar population. The galactic disk appears relatively smooth, with a hint of bluer light extending from the central bulge along the major axis, suggesting some ongoing star formation. There is no apparent evidence of a major merger event or strong tidal disturbances, although a minor irregularity is present on the top of the galaxy which indicates there may have been a minor merger. The galaxy's overall morphology suggests a significant degree of rotational symmetry.
