This galaxy presents as an edge-on spiral system. A prominent, centrally concentrated bulge exhibits a yellow-orange hue, suggestive of an older stellar population. The disk component appears thin and elongated, with hints of bluish regions along the edges, potentially indicating zones of active star formation. There is no obvious major disturbance in the galaxy's morphology; however, there might be minor asymmetries that could suggest minor interactions or internal dynamics within the disk. The bulge appears somewhat boxy in shape, and there may be a dust lane bisecting the galaxy, though its presence is only weakly suggested by a slight darkening in the central regions. The overall form is smooth, with low levels of granularity.
