The galaxy is a spiral type, exhibiting a clear disk structure. Two prominent spiral arms are visible, winding moderately around a central bulge. The bulge appears to be of moderate size relative to the disk. There's a suggestion of a bar-like structure bisecting the bulge, extending into the inner regions of the spiral arms. The spiral arms display subtle color variations, hinting at ongoing star formation regions interspersed along the arm structure. The disk itself shows a slight inclination relative to our line of sight, offering a partial view of its three-dimensional structure. The overall morphology suggests a relatively undisturbed galaxy, without signs of major mergers or tidal disruptions. The core is bright, which can mean that the Black hole in the center has high activity.