The galaxy presents a primarily blue hue, suggestive of ongoing or recent star formation. Its morphology is elongated and irregular, possibly indicating a disturbed structure. There appears to be a brighter, concentrated central region that could represent a galactic nucleus or a region of particularly intense starburst activity. Fainter, diffuse extensions extend outwards from the central region, hinting at tidal features or disrupted arms. The shape could suggest an ongoing or recent merger event. Overall, the galaxy appears to be a relatively compact system with evidence of significant star formation and potential dynamical disturbances.
