The galaxy presents as a somewhat elliptical object, with a major axis extending roughly northeast to southwest. Its core exhibits high luminosity, appearing bright and nearly spherical. Fainter, diffuse extensions emanate outwards from the central region, with the southern extension appearing more prominent than that on the northern side. The overall color appears slightly redder in the outer regions, which may indicate the presence of older stellar populations compared to the brighter core. A possible secondary concentration of light, slightly less luminous than the core, can be observed to the northeast. This could be the result of a galaxy merger. The galaxy appears fairly smooth in texture with little to no evidence of spiral arm structures or prominent dust lanes.
