The observed galaxy presents as an elongated structure with a noticeable disk component. It is likely an edge-on spiral galaxy. The central bulge exhibits a yellow-orange hue, suggestive of an older stellar population and/or dust obscuration. The outer disk appears bluer, potentially indicating younger, hotter stars and ongoing star formation. The disk appears relatively smooth, without prominent spiral arm features visible. There are some hints of subtle disturbances, like the disk appears slightly warped. The morphology of this galaxy appears primarily undisturbed.
