This galaxy presents as an edge-on spiral, or possibly lenticular, system. It exhibits a prominent, elongated central bulge, appearing yellowish in color, which suggests an older stellar population. The disk is observed nearly edge-on, showing a slight warping. There is evidence of some structure within the disk, but no distinct spiral arms are discernible. The overall color of the disk appears bluer than the bulge, indicating the presence of younger stars and potentially some ongoing star formation. There are no signs of a major merger event or strong tidal disturbances. The morphology indicates that this galaxy is more likely to be an edge-on spiral.
