The galaxy presents as a relatively compact object with a smooth, diffuse appearance. Its color suggests a population of older stars, possibly with ongoing, but limited star formation, giving it a slightly bluer tinge. The morphology appears roughly elliptical or spheroidal with a generally round structure, showing no strong indications of spiral arms or a prominent disk. There are hints of minor disturbances or irregularities in its shape and light distribution but these are quite faint, potentially indicating past or ongoing weak interactions. The overall structure suggests it is likely a galaxy with a modest stellar mass and a low star formation rate.
