The galaxy presents as a generally smooth, elongated object. It exhibits a somewhat cigar-shaped morphology, lacking a prominent, well-defined spiral structure. The central region displays a brighter, more concentrated luminosity, suggesting a central bulge. There is a slight asymmetry in the galaxy's structure. One end shows a small, reddish extension, potentially indicating an area of active star formation or possible tidal disruption. The overall color is bluish-white in the central region, suggestive of a younger stellar population, while the outer regions are fainter and appear redder. There's a slight indication of minor disturbances or possible interactions, but it does not seem to be a major merger event.
