The galaxy appears as a relatively small, well-defined elliptical structure. It presents a centrally concentrated morphology with a smooth light distribution, showing no apparent spiral arms or distinct features indicative of a disk galaxy. The color profile seems to be a relatively uniform cyan, suggesting a population of stars emitting strongly in the green and blue wavelengths. There is a slightly redder core region, which is consistent with the presence of older stellar populations or dust. There are no obvious signs of active galactic nuclei or ongoing star formation regions. The overall symmetry is perturbed by the presence of a slight asymmetry to the lower right, and a possible minor disturbance in its overall shape, hinting at a possible past or ongoing interaction, or some internal activity.
