The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. It displays a concentrated central bulge that gradually diffuses into an extended halo. There is some evidence of a faint disk-like structure surrounding the bulge, but it lacks defined spiral arms. The galaxy presents a yellow to white hue, suggestive of a population dominated by older stars, with very little or no active star formation apparent. No signs of tidal disturbances or ongoing mergers are immediately noticeable. It exhibits a rounded morphology.
