The galaxy presents as a faint, diffuse object with a subtly elongated morphology. There is no distinct nucleus, and the light appears broadly distributed. Overall, the galaxy seems to lack a coherent structure. Faint hints of possible tidal features, or minor disturbances, appear to extend outward from the central body in different directions. These potential features are difficult to discern due to their faintness and the low resolution. The galaxy exhibits a color gradient; The central region appears redder in comparison to the outer edges, which appear bluer. This could indicate differing stellar populations with older stars concentrated in the center, or a differential distribution of dust.
