The galaxy presents as a somewhat elongated, diffuse object. Its overall color appears bluish, suggesting the presence of relatively young stars. The central region exhibits a brighter, more concentrated luminosity, possibly indicating the presence of an older stellar population or an active galactic nucleus. A slight asymmetry can be observed in the outer regions, potentially suggesting past or ongoing gravitational interactions with another galaxy. The galaxy's morphology is somewhere between round and cigar shaped and the galaxy exhibits minor disturbances. The central regions are more red than the peripheral regions, which suggests a more active region or recent burst of star formation.

The galaxy's features point towards a possible recent merger event or active galactic nucleus in the center. Further spectroscopic analysis is warranted to confirm these hypotheses.
