The galaxy presents as a single, relatively smooth object. It exhibits an elliptical morphology with a dominant, centrally concentrated bulge. The light profile appears to decrease smoothly from the center outwards, with no distinct spiral arms or bar structure visible. The color is predominantly yellowish-white, suggesting a population of older stars with moderate ongoing star formation activity. There is little evidence of significant dust lanes or prominent HII regions. The overall appearance suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy viewed close to face-on. There may be some minor disturbance in the symmetry of the galaxy, which suggests a possible past interaction with another galaxy.
