The galaxy presents as a single, luminous object, displaying a generally smooth morphology. There may be some indication of substructure within the galaxy's overall form, but the resolution does not allow for a definitive determination. Color gradients are subtle, but the central region appears slightly more concentrated in redder wavelengths, suggesting a possible concentration of older stellar populations toward the core. The galaxy's light profile is quite diffuse, indicative of a lack of distinct spiral arms or a prominent galactic disk. The overall shape of the galaxy appears generally circular. There is some indication of a minor gravitational disturbance.
