The galaxy presents as a fairly smooth, centrally concentrated object. Its light profile suggests a spheroidal morphology, with a dominant bulge component and a lack of discernible spiral arm structure. The color appears generally redder, indicating an older stellar population and relatively low levels of ongoing star formation. The overall shape is close to round, with no obvious signs of significant tidal disturbances or ongoing mergers. There is a slight elongation visible, though it is subtle. The galaxy appears relatively isolated, with no other nearby galaxies visibly interacting with it. Based on these characteristics, the object is most likely an elliptical galaxy at a considerable distance.
