The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The light from the core appears yellowish, possibly indicating an older stellar population. The outer regions of the galaxy exhibit a bluer hue, hinting at the presence of younger, hotter stars and ongoing star formation. The overall smoothness of the light distribution suggests that this galaxy is relatively undisturbed, lacking prominent spiral arms or significant dust lanes. However, there is a subtle irregularity in the galaxy's shape. The galaxy's moderate redshift implies that it is at a significant cosmological distance.
