The galaxy appears to be in a state of interaction, possibly a merger. The central region shows a concentrated, bright core, with evidence of significant star formation. The galaxy exhibits a disturbed morphology, lacking a clear, defined structure. There are hints of tidal tails or extended features, though the image resolution limits detailed analysis. The color distribution is uneven, with a dominant yellowish hue mixed with redder patches near the central area, indicative of dust and ongoing star formation. Overall, the galaxy presents as a complex system undergoing dynamic processes.
