The galaxy presents as a moderately concentrated system, exhibiting a slight ellipticity. Its color appears generally blue-white, suggesting a population of younger, hotter stars and ongoing star formation. There is an indication of some structural disturbance, as the morphology is not perfectly smooth or uniform. A faint halo or extended stellar component may be present, but the image resolution limits detailed analysis. The galaxy does not appear to be undergoing a major merger event, but it does have faint signs of minor disturbances or tidal interactions. Its apparent size is small, which, combined with its redshift, indicates that we are observing this galaxy at a significant distance. Overall, it is likely a spiral or an irregular galaxy.
