The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a notable concentration of light, appearing relatively smooth. Towards the periphery, specifically along one edge, there is evidence of fainter disk features or potential tidal disturbances, which seem to be interacting with a neighbor galaxy. The color profile suggests a mix of stellar populations; the central bulge appears redder, indicating older, less active star formation, while the disk contains bluer components, suggesting the presence of younger stars and ongoing star formation. There is possible evidence of disruption in its spiral structure on its right side. Overall, the galaxy appears to be a relatively massive system with ongoing processes.
