The galaxy presents as a singular, relatively smooth object with an approximate angular radius of 1.8 arcseconds. The morphological classification appears to be trending towards elliptical, based on its rounded appearance. There is a lack of defined spiral arms or a distinct disk structure. The galaxy does not appear to be undergoing any major merging events, although a slight asymmetry is present, potentially indicative of a minor interaction or internal disturbance. The central bulge region is not overly prominent, and the galaxy appears relatively uniform in color and intensity across its visible surface.
