The galaxy appears as a relatively smooth, elliptical or lenticular object. It exhibits a concentrated central bulge that dominates its overall light profile. The galaxy appears highly circular, lacking any obvious spiral arm structure or significant morphological disturbances indicative of recent major mergers. There is an absence of significant dust lanes or patchy star formation regions. The overall color is suggestive of an older stellar population with a lower rate of ongoing star formation. It is moderately luminous and appears to be a substantial galaxy, given its redshift. No evidence of active galactic nuclei activity can be determined.
