The galaxy presents a generally disk-like morphology, observed at an oblique angle, neither perfectly face-on nor edge-on. The central region is noticeably brighter and appears to be undergoing significant activity, possibly related to an active galactic nucleus or enhanced star formation. The galaxy exhibits a blue hue, suggesting the presence of a relatively young stellar population and ongoing star formation. Evidence of a possible ongoing or recent merger event is indicated by the irregular shape and the presence of tidal tails or disrupted arms extending outwards from the main body. These features are more prominent on one side of the galaxy, further suggesting an asymmetrical interaction. Overall, the galaxy appears to be a dynamically active system with ongoing star formation and evidence of interactions.
