The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a generally elliptical shape, showing a high degree of roundness. There is little visual evidence of a prominent disk structure or spiral arms, suggesting that it is more likely an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy's color is noticeably blue-white, implying the presence of a younger stellar population and possible ongoing star formation, though the overall smoothness suggests that this may not be occuring at a very high rate. There is no immediately visible evidence of any major ongoing merger activity or significant tidal disturbances. Slight color variation in the outskirts could indicate some substructure or differential star formation, but overall the structure presents a homogenous appearance.
