The galaxy presents as a disk galaxy, viewed nearly edge-on from our line of sight. There is a noticeable bulge; it appears somewhat rounded. There is no obvious sign of significant tidal disruption or major merger activity. The galaxy exhibits a relatively high level of star formation. The disk appears to have a yellow/white hue. This suggests an intermediate population of stars. The disk itself shows some signs of patchy structure, possibly due to dust lanes or regions of varying stellar density. The overall morphology suggests a spiral galaxy, potentially a late-type spiral, with a notable disk structure and central bulge.
