The galaxy presents as a spiral structure with well-defined arms. There is a bright, concentrated central bulge that appears yellowish. The spiral arms exhibit a bluer hue compared to the bulge, suggesting the presence of younger stellar populations. The arms are tightly wound around the galactic center. The galaxy has a high degree of rotational symmetry, with a relatively undisturbed disk. The overall morphology is characterized by a prominent disk component and a moderate bulge. There is no strong evidence of significant ongoing mergers or tidal interactions. The disk is viewed at a shallow inclination. The overall appearance suggests a galaxy in a relatively quiescent state of evolution.
