The galaxy appears relatively compact, displaying a concentrated central region. Its overall structure seems largely smooth, with a noticeable lack of defined spiral arms or a prominent disk component. There is a slight asymmetry in its light distribution, suggesting a possible disturbance. Color variations are present, with the core appearing a lighter shade in comparison to the outer edges. Upon closer inspection, a hint of tidal features can be tentatively identified, potentially indicating minor gravitational interaction with another galaxy or object in the distant past.
