The galaxy presents a morphology that appears primarily smooth, though some underlying features suggest a disk-like structure. It exhibits an approximate circular shape with moderate ellipticity. There is little indication of strong spiral arms or a prominent bar structure. The color profile is suggestive of an aging stellar population, with a yellow-orange hue dominant in the central region that slightly fades to a pale yellow toward the edges. The outer regions show hints of some blue features. There is no obvious sign of a major ongoing merger. Minor disturbances could be possible, based on the slightly asymmetrical distribution of light, but such disturbances are faint. Overall, the galaxy appears to be a relatively quiescent system, possibly in a later stage of its evolution.