The observed galaxy presents as a disk galaxy, viewed at a near edge-on orientation. A distinct bulge is visible, appearing somewhat yellow in color, suggesting a population of older stars within. The disk shows evidence of spiral structure, though it is not sharply defined. Dust lanes appear present, obscuring parts of the disk. The overall color of the disk is bluer compared to the bulge. The galaxy appears to be relatively isolated, showing no obvious signs of recent major merger activity, although there may be some minor tidal disturbances or asymmetries within the disk. The size of the galaxy suggests that it is a fairly massive object. There is ongoing star formation.