The galaxy presents as a moderately bright, compact object. Its overall morphology appears largely smooth, with a concentrated central region of relatively high surface brightness. There is some evidence of extension or perhaps faint, diffuse structure surrounding the central region. The color appears to be mostly yellow to golden, suggesting a population of older stars, but there are also blue hues mixed into the galaxy's color, indicating the presence of some younger stars. There may be slight perturbations to the overall shape. A small fraction of the galaxy's light shows evidence of disruption or merger activity. The overall structure seems somewhat disturbed.
