The galaxy presents as a disk-shaped structure, viewed edge-on. A prominent bulge is observed, exhibiting a concentrated, yellowish-white hue indicative of an older stellar population. The galactic disk is elongated, displaying a significant degree of flattening. Faint blue regions can be discerned extending along the outer edges of the disk, suggesting areas of recent star formation. There is no obvious spiral arm structure to the disk, suggesting a relatively smooth, less structured distribution of stellar material. The galaxy exhibits a relatively small angular size, suggesting a large distance from us. No distinct dust lanes are apparent within the disk. Overall, the galaxy appears to be an edge-on spiral or lenticular galaxy with a prominent bulge and some ongoing, but limited, star formation within the disk.
