The galaxy presents as a fairly smooth, unresolved object with a slightly elliptical morphology. It exhibits a central concentration of light, suggesting a bulge component. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy's color appears relatively uniform, trending towards the redder end of the spectrum. This implies an older stellar population and relatively low ongoing star formation. There is a slight indication of some minor disturbance in the symmetry, which could be from a past interaction with another galaxy.
