The galaxy appears to be an elongated, cigar-shaped structure. A central, brighter region shows a yellowish hue, potentially indicating an older stellar population or dust obscuration. Emanating from this region is a bluer component, possibly indicative of more recent star formation. It seems this bluer area is separate from the main galaxy. The galaxy exhibits signs of possible tidal disturbance or interaction, showing minor disruptions in its form. There is evidence of a merging event that is in progress.
