The galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy viewed nearly edge-on. The central region exhibits a concentrated luminosity with a yellowish hue, possibly indicating an older stellar population within the bulge. Diffuse, bluer light extends from the central region along the major axis, which is indicative of ongoing star formation in the galactic disk. There's a subtle indication of dust obscuration in the disk. The morphology suggests the galaxy is relatively undisturbed, with no signs of a recent major merger.