The galaxy presents as an elongated, cigar-shaped structure. It exhibits a generally smooth morphology, with no readily apparent spiral arms or distinct features beyond a central bulge. The light distribution within the galaxy is concentrated toward the center, gradually decreasing outwards. There is a slight color gradient, with the central region appearing somewhat redder compared to the outer regions which are slightly bluer. This color variation might indicate differing stellar populations or dust distribution within the galaxy. There is no evidence of any ongoing mergers or major disturbances in the galaxy's structure.
