The galaxy appears as an elliptical or lenticular system, characterized by a relatively smooth and centrally concentrated light distribution. The core region exhibits a bright, diffuse glow. Moving outward, the light fades gradually into the surrounding space. There is a hint of bluer light that might be interpreted as a disk-like structure or spiral arms. The galaxy shows no signs of major disturbances or tidal tails, indicating that it is not undergoing a major merging event, although there is a slight asymmetry that may indicate a minor past interaction. Based on the apparent color distribution, the galaxy likely has a moderate amount of star formation present. Overall, the galaxy presents itself as a fairly evolved system.
