The galaxy appears as a somewhat elliptical, disk-like structure. It exhibits a smooth, centrally concentrated bulge that transitions into a flattened disk. The color gradient suggests a composition of older stars within the central bulge, indicated by the yellowish hue, and slightly bluer regions within the disk component, possibly indicative of ongoing, yet weak, star formation. There are no distinct spiral arms visible, though subtle variations in color and density may suggest underlying disk structure. Overall the galaxy presents as a relatively undisturbed system, with no clear signs of major mergers or significant tidal interactions. The disk is moderately inclined to our line of sight, lending it an elongated appearance. 
