The galaxy presents as an elliptical-like morphology, exhibiting a smooth, diffuse light profile. There is no discernible spiral arm structure or distinct nucleus. The light distribution appears relatively even throughout the galaxy's extent. The galaxy exhibits a somewhat spheroidal shape, showing no clear elongation, or significant deviation from circularity. The core regions are brighter with an orange-yellow hue, and that color fades to green at the outer edges. I observe subtle irregularities in the galaxy's outer regions, suggesting possible minor disturbances or interactions. Overall, the galaxy appears to be relatively isolated and undisturbed.
