The galaxy presents as a single, relatively smooth object with an overall elongated, cigar-shaped morphology. It appears to lack any distinct spiral arm structures or prominent dust lanes. The light is centrally concentrated with a diffuse, fading luminosity gradient extending outwards from the core. There is a subtle color gradient across the galaxy, with the core exhibiting a bluer hue and the outer regions trending slightly redder. There are no obvious signs of any major mergers or tidal disturbances, though some minor asymmetry cannot be ruled out. The galaxy does not present with obvious star forming regions and its stellar population appears generally old.
