This galaxy presents an overall smooth morphology, appearing relatively undisturbed. The light distribution indicates a centrally concentrated structure. Color gradients are present, transitioning from a bluer hue towards the outer regions to a redder hue in the core, suggesting differing stellar populations and/or dust distribution within the galaxy. The galaxy is fairly round in appearance, showing a lack of defined spiral arms or a prominent disk. There is no apparent ongoing merger activity, although the system is not perfectly uniform, exhibiting some asymmetries. The moderate redshift suggests that we are observing this galaxy at a significant cosmological distance.
