The galaxy appears to be a spiral galaxy seen edge-on. It exhibits a prominent central bulge with a yellowish hue, indicative of an older stellar population. The disk is elongated and displays a bluish-white color, suggesting the presence of younger, hotter stars. The galaxy's morphology is somewhat irregular, with a slight warp or asymmetry visible in the disk. There are no clear signs of a major ongoing merger, though some minor disturbances may be present. Overall, it is a substantial galaxy, with a relatively high mass and moderate levels of star formation.
