The galaxy presents as a spiral system, viewed at an oblique angle, close to edge-on. The central bulge appears moderately prominent, exhibiting a yellowish hue, suggesting an older stellar population. Faint spiral arms extend outward from the bulge, displaying a bluer tint indicative of more recent star formation. These arms are somewhat flocculent in nature, lacking a grand, well-defined design. There's a noticeable dust lane running along the major axis, obscuring the light from the bulge and contributing to the reddening of the central region. The overall shape of the galaxy is elongated, consistent with an elliptical projection due to the viewing angle. No signs of any major merger events are immediately apparent, however some asymmetry is noticed in the dust lane.
