The galaxy presents as a disk-shaped structure, observed at an oblique angle. It exhibits a prominent central bulge, characterized by a yellowish-white hue, suggestive of an older stellar population with lower rates of star formation. The disk component shows a less distinct spiral arm structure, appearing somewhat flocculent. The outer regions of the disk gradually fade into the background, with an overall smooth appearance. There are hints of blueish regions embedded in the disk, possibly signifying areas of more active star formation. The galaxy seems relatively isolated, showing no obvious signs of recent major mergers or strong tidal interactions with neighboring galaxies. Minor asymmetries or disturbances in the outer disk could point to some interaction. The galaxy's intermediate roundedness suggests a transition between a spheroidal and a flattened morphology. 
