The galaxy presents a yellowish hue in the central region, suggesting an older stellar population. The light is concentrated, giving off a impression of relatively high density of stars. There is a structure that looks like a disk, with the yellowish central region fading into a less concentrated blueish light. The disk shape is distorted in the direction of the bottom left, with a tail of lighter luminosity. This could indicate a tidal interaction or ongoing minor merger, though the primary body of the galaxy seems relatively undisturbed. Overall, the morphology indicates that it is likely an early-type spiral galaxy undergoing a merger.
