The galaxy presents as a disk galaxy, viewed nearly edge-on from our line of sight. A prominent central bulge is visible, exhibiting a roughly spheroidal morphology. The color of the bulge appears redder than the surrounding disk, potentially indicative of an older stellar population within the bulge. 

The galactic disk appears relatively thin and elongated, characteristic of edge-on spiral or lenticular galaxies. Some degree of substructure, potentially representing dust lanes or spiral arm segments, can be inferred along the length of the disk, though the resolution is not sufficient for detailed analysis. The disk exhibits a bluer color gradient than the bulge, suggestive of ongoing star formation activity. No obvious signs of significant tidal distortion or major merger activity are apparent, though minor disturbances cannot be ruled out based on this image alone. The apparent axial symmetry and lack of significant asymmetries support a classification as a relatively undisturbed disk galaxy.
