The galaxy presents as a somewhat elliptical, though nearly round, structure. There's a distinct color gradient across the galactic disk, suggesting variations in stellar populations or dust content. One side appears bluer in hue, possibly indicative of ongoing star formation or a population of younger, hotter stars. The opposite side exhibits a more yellow to reddish color, which could suggest an older stellar population or the presence of dust obscuring bluer light. There is some potential evidence of minor disturbances. There is some possibility of a merging event but it is difficult to discern. Based on the smoother appearance, it may be an early stage of galaxy evolution, such as an elliptical or lenticular galaxy.
