The galaxy presents as a disk-shaped structure, with a distinct central bulge. The bulge exhibits a yellowish hue, potentially indicative of an older stellar population. The disk is oriented at an angle to our line of sight. A subtle color gradient is observed within the disk, transitioning from a greenish-blue closer to the core to a slightly redder hue in the outer regions. The galaxy appears relatively undisturbed, displaying a smooth and regular morphology. No prominent tidal features or signs of recent major mergers are immediately apparent. There is a possibility of minor disturbances or slight asymmetries in the outer disk regions.
