The galaxy presents as a moderately inclined, disk-shaped system. Its overall color is indicative of a population of older stars, though the presence of some bluer regions suggests ongoing or recent star formation. The galaxy exhibits a smooth light profile, hinting at a dominant bulge component. No significant signs of strong spiral arm structure are clearly visible, nor is there a clear indication of a prominent bar structure. The disk appears relatively undisturbed, showing no strong tidal features, asymmetries, or evidence of recent major merger events. The ellipticity measurements suggest that the galaxy is not viewed perfectly edge-on, but at a moderate angle.
