The object presents as a galaxy with an apparent redshift. It displays a centrally concentrated luminosity profile, suggesting a relatively smooth morphology. The galaxy appears nearly circular. The image does not resolve any distinct spiral arms or a prominent disk structure. The galaxy exhibits a color gradient, with a slightly redder core region transitioning to bluer outer regions. There is no obvious indication of a major ongoing merger. However, subtle irregularities in the outer halo might be indicative of minor gravitational disturbances or past interactions. The galaxy is relatively massive. It seems to be actively forming stars, albeit at a modest rate.
