This galaxy appears as a slightly elongated, smooth structure with a dominant central bulge. The light distribution indicates that it is most likely an elliptical galaxy or a lenticular galaxy viewed at an angle. The colors suggest an older stellar population, primarily composed of redder stars, as expected in such galaxies. There are subtle variations in color across the galaxy, which could indicate differences in stellar populations or dust distribution, but the resolution is insufficient to resolve individual structures or star-forming regions. Overall, the galaxy presents a relatively undisturbed morphology. There are no obvious signs of spiral arms or a disk. There is possibly another galaxy it is interacting with, or a star cluster near it.
