The galaxy presents as a relatively small, disk-shaped structure seen nearly edge-on. A bulge is apparent within the center, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. Fainter, bluish light extends outwards from the bulge along the disk, suggesting the presence of younger, hotter stars and ongoing star formation. The overall morphology appears smooth, but slight asymmetry in the distribution of the bluer regions may indicate minor disturbances or interaction with another galaxy. The galaxy doesn't appear to be undergoing any major merger activity based on the image. The disk itself appears relatively thin.
