This galaxy appears to be a spiral galaxy viewed nearly edge-on. A prominent, rounded bulge dominates the central region, displaying a smooth and concentrated luminosity profile. The disk component of the galaxy is visibly flattened and extends outwards from the bulge. There is evidence of possible internal dust lanes obscuring the bulge. The blue hues at the edge of the galaxy may suggest regions of ongoing star formation. Overall, the galaxy's morphology seems relatively undisturbed, with no obvious signs of major recent merger activity.
