The galaxy appears as a centrally concentrated object exhibiting a smooth, diffuse light profile, with a hint of a flattened shape reminiscent of a disk. The galaxy's color is predominantly blue, suggesting a population of relatively young, hot stars and ongoing star formation. Though smooth, some minor disturbances or irregularities in the outer regions suggest potential past interactions, or perhaps internal activity. The bulk of its mass resides in its inner regions and is not experiencing any major mergers. The overall morphology indicates an intermediate state, leaning towards spheroidal but retaining some disk-like characteristics, with the majority of the mass not undergoing major star formation.