The galaxy presents as a complex system exhibiting signs of interaction or recent merger activity. A prominent, relatively smooth, central component displays a yellowish hue, possibly indicating an older stellar population. Arcing away from this central region is a bluish structure, suggesting ongoing or recent star formation. The main body of the galaxy appears somewhat elongated, neither perfectly spherical nor highly flattened. Faint tidal features, perhaps faint streamers or tails, are suspected in the diffuse outskirts of the system. There are a few smaller, less distinct clumps of light in the vicinity which may be smaller interacting galaxies. Overall, the system shows signs of significant gravitational disturbance.
