The galaxy is lenticular in appearance, exhibiting a smooth, elongated structure. A bright, concentrated central bulge is visible, suggesting a significant population of older stars. Fainter, bluer light is present in what appears to be a flattened disk, indicating regions of possible ongoing or recent star formation. The galaxy's overall color suggests it is a mature system with a mix of stellar populations. There is no indication of any active galactic nucleus. The general morphology indicates a system that has largely exhausted its gas supply, slowing down star formation, and is not currently undergoing any major merging events.
