The galaxy presents as a slightly inclined disk galaxy, approximately 7 kpc in diameter, oriented along its major axis. The central bulge region appears bright and yellow-white in color, indicating an older stellar population. A faint, bluish disk surrounds the bulge, suggesting the presence of some younger, star-forming regions. There is also evidence of dust lanes within the disk, visible as subtle dark patches silhouetted against the brighter regions. These dust lanes appear most prominent along the plane of the disk. The outer edges of the disk exhibit a flocculent structure, indicating that the galaxy is not a grand design spiral. The galaxy shows no signs of major merger activity, but may have experienced some recent minor disturbances, judging by the patchiness of the disk. Overall, the galaxy appears to be a relatively quiescent system, with a moderate amount of star formation activity.
