The galaxy presents as a relatively smooth, centrally concentrated object. The morphology leans toward elliptical, with a high degree of roundness observed. There's a slight indication of a possible minor disturbance or interaction. The galaxy exhibits color variations, shifting from bluer hues in what appears to be one region to redder tones in another, perhaps indicating differing stellar populations or dust content within the system. Though seemingly a single galaxy, this color variation suggests it may in fact be two galaxies in the process of merging, explaining the disturbance. The object's luminosity is consistent with a moderately massive galaxy.
