The observed galaxy presents as an elliptical-like morphology, exhibiting a smooth, concentrated distribution of light. The galaxy appears largely featureless, lacking discernible spiral arms or significant dust lanes. The light profile suggests a central bulge that dominates the galaxy's luminosity. A slight elongation can be observed, deviating from a perfect circular shape; the galaxy can be described as slightly oblong. There is a color gradient observed, where the central region is more yellow in appearance than the light at the edge of the galaxy, which has a more reddish hue. There appears to be no current merging activity.
