The galaxy presents as a relatively small, elongated system. Its morphology appears predominantly smooth, lacking prominent spiral arms or a well-defined disk structure. The central region exhibits a noticeable concentration of light, possibly indicating a bulge component. The color profile suggests a redder core transitioning to bluer outer regions, potentially indicative of differing stellar populations, with older, redder stars concentrated centrally and younger, bluer stars towards the periphery. Overall the light is fairly dim indicating that there is low star formation occurring. The smooth appearance suggests a potential classification as an elliptical galaxy, or possibly a lenticular galaxy viewed edge-on. There are no signs of major disturbances, like tidal tails or multiple nuclei, which suggests it has not recently merged with another galaxy. The shape appears very elongated, like a cigar.
