The galaxy presents as a smooth, elongated structure with a high degree of axial ratio. There is no discernible spiral arm structure, but some slight bluing is evident at the edges. The central region exhibits a higher surface brightness, fading outwards. There are no obvious signs of ongoing major merger activity or tidal features, but some minor disturbances may be present. The overall color index suggests a population of older stars, though some ongoing star formation may be present in the outer regions. It likely resides at a distance where 1 arcsecond subtends approximately 2 kpc.
