The galaxy presents a largely smooth morphology with a concentrated central bulge, indicative of an elliptical or lenticular type. The light distribution appears relatively even, suggesting an older stellar population with minimal ongoing star formation, supported by a high mass estimate but low star formation rate. The object exhibits a generally rounded shape with a slight elongation visible along one axis. There are no obvious signs of spiral arms or significant dust lanes. The overall color is reddish, possibly resulting from redshift, suggesting this galaxy is a considerable distance away. There is no indication of any major merging activity or significant tidal disturbances in its immediate environment, although minor disturbances or a previous merger cannot be ruled out from this image alone.
