The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a bright, concentrated luminosity, suggesting a substantial stellar population or potentially an active galactic nucleus. The light appears to be redshifted towards the redder end of the spectrum. There is likely ongoing star formation activity within the galaxy. No distinct spiral arms or bar structures are discernible within the galaxy. There is no clear visual indication of significant tidal disturbances or major merger events, yet some asymmetry is present.