The galaxy presents as a relatively smooth, centrally concentrated object, with no obvious spiral arm structure visible. Its overall shape appears somewhere between round and elliptical. The galaxy displays a color gradient, with a somewhat bluer central region transitioning to redder hues in the outer parts. There's no strong evidence of tidal tails or significant morphological distortions suggesting recent major merger activity; however, there may be very subtle signs of minor disturbance in the outer regions. The central region exhibits comparatively bright emission. Overall, the galaxy appears to be a system with modest ongoing star formation, with a mass that is relatively typical for galaxies in the observed redshift range.
