The galaxy appears to be a relatively smooth, centrally concentrated object with a slightly elongated morphology. The light distribution suggests a dominant bulge component, possibly indicative of an elliptical or lenticular galaxy type. Faint blue emission is visible, particularly on the outer edges, which may indicate a low level of on-going star formation, primarily in the disk region. There are no obvious signs of strong tidal interactions or major mergers; however, a possible minor disturbance can not be ruled out. The galaxy has an apparent magnitude that suggest it is a luminous object given its redshift. Overall, this galaxy exhibits characteristics of a well evolved galaxy with a mix of old stellar populations and some current star formation.
