The galaxy appears to be an elliptical galaxy, or possibly a lenticular galaxy viewed at an angle. It has a smooth, diffuse structure with a concentrated central bulge. The color gradients suggest a population of older stars, exhibiting a redder hue toward the outer regions. There are no obvious spiral arms or significant dust lanes visible. The galaxy appears largely undisturbed, without major signs of ongoing mergers or interactions, although there is a slight elongation and a potential minor disturbance in its morphology. The overall light distribution indicates a relatively high degree of symmetry. The galaxy has a relatively high luminosity.
