The galaxy presents a largely smooth morphology with some evidence of internal structure. It exhibits a moderate degree of ellipticity, appearing somewhat elongated rather than perfectly circular. There is a color gradient visible, transitioning from a redder core region to slightly bluer, but still faint, outer regions. The galaxy displays a faint disk-like structure which could imply ongoing, although likely weak, star formation activity. This interpretation of the galaxy suggests that it likely contains a significant population of older stars and could be a post-starburst or passive galaxy. The size suggests it is a relatively large galaxy. Based on the light, this galaxy seems like it is in a relatively isolated environment, with no apparent major merging events or tidal disturbances influencing its structure.
