The galaxy presents a moderately bright, centrally concentrated morphology. It appears largely smooth in structure, though there are suggestions of some internal features, possibly faint spiral arms or dust lanes, but these are not sharply defined. The overall shape is somewhat elliptical, exhibiting a mild elongation. Color gradients across the galaxy are subtle. The central region is slightly bluer than the outer regions, suggesting the possibility of ongoing star formation, although at a low rate. The galaxy does not appear to be undergoing any major merger events or tidal disturbances.
