The observed galaxy presents as an elongated, likely disk-shaped structure viewed nearly edge-on from our perspective. The central region exhibits a higher concentration of luminosity, appearing yellowish, possibly indicative of an older stellar population or significant dust obscuration. Progressing outward from the core, the light gradually diffuses into a fainter, bluer haze, suggesting a younger stellar population within a more extended disk. There is no immediately apparent grand design spiral structure, nor are there any signs of ongoing major merger events. The morphology seems relatively undisturbed, with only subtle indications of minor asymmetry or tidal features. The disk appears quite thin, and there's a slightly boxy shape to the bulge.
