The galaxy appears to be a relatively smooth and rounded system. The central region exhibits a distinct yellowish hue, suggesting a population of older stars. Moving outward from the core, a more diffuse, bluish halo can be observed, possibly indicating the presence of some younger stellar populations or ongoing star formation, albeit at a relatively low rate. There may be slight asymmetries or subtle disturbances in the outer regions of the galaxy, but no significant signs of major mergers or interactions are visible. The morphology suggests a transition between an elliptical and a spiral galaxy.