The galaxy presents as a relatively compact, disk-shaped structure. The light distribution indicates a bulge component, although it appears small and not particularly prominent. The overall color suggests it may be in the green valley. The color gradient indicates the presence of ongoing star formation, but may be beginning to fade, as it exhibits a relatively modest star formation rate. The galaxy's morphology is somewhat smooth, though with a subtle underlying disk-like structure. There are no obvious signs of strong tidal interactions or major mergers, though there might be some disturbance of the galaxy that could possibly be caused by a minor merger. No clear spiral arm structures are observed, it appears mostly as a disk with a small bulge. The galaxy appears highly inclined, with it's disk appearing edge-on from our vantage point.
