The galaxy presents a relatively smooth morphology, with a hint of a disk-like structure. The central region appears more concentrated and brighter, suggesting the presence of a bulge. There are subtle irregularities in the outer regions, possibly indicating minor disturbances or interactions. The overall color is slightly blueish, suggesting the presence of some younger stars and ongoing star formation, although potentially at a low rate. No strong evidence of a major merger is apparent, but the asymmetry of the outer disk warrants further investigation for signs of past interactions. The galaxy appears moderately compact.
