The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is elongated, displaying an apparent cigar-like morphology. The central region exhibits a concentration of light, suggestive of a bulge component. Fainter light extends outwards from the central bulge, fading gradually into the surrounding space. There is no obvious spiral arm structure or distinct features such as dust lanes are observed. The galaxy is primarily yellowish-white in color, with perhaps a slight blue tinge on the outer edges, indicative of the presence of younger stars. There are no visible signs of a major ongoing merger, although subtle irregularities might indicate a minor disturbance in the system's recent history.
