The galaxy presents as an edge-on spiral, exhibiting a flattened, disk-like morphology. The galactic bulge is prominent, displaying a notably rounded shape. The disk appears relatively smooth with no visible arm structures, obscuring inner structures. The galaxy exhibits an apparent reddish hue, suggestive of an older stellar population. There is little evidence of recent or ongoing major mergers, though subtle morphological disturbances cannot be entirely ruled out.
