This galaxy presents as a well-defined, disk-shaped structure. The central region displays a bright, concentrated bulge, transitioning outwards into a more diffuse disk. A subtle hint of spiral structure is apparent within the disk, indicated by a slight swirling pattern. The galaxy exhibits a color gradient, with the central bulge appearing yellower in comparison to the bluer hues in the outer disk. This color variation suggests a population of older stars towards the center and younger, bluer stars dominating the spiral arms. The overall impression is that of a galaxy undergoing moderate star formation. There are no strong indications of any major mergers or significant disturbances. The morphology appears generally smooth, without any large tidal tails or bridges.
