The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a slightly elliptical morphology, with a high degree of roundness but not perfectly circular. A bright, yellowish core dominates the galaxy's appearance, suggesting a significant population of older stars. Fainter, diffuse light extends outward from the core, with subtle color gradients indicating varying stellar populations. The overall structure shows little evidence of strong spiral arms or significant disturbances, suggesting it might be a fairly evolved system. There is some evidence of a slight perturbation on the lower left of the galaxy, but no major merging event is apparent.
