The galaxy presents a generally smooth, rounded morphology. The light is relatively concentrated towards the center, suggesting a significant bulge component. The overall color appears somewhat redder, implying a stellar population that is dominated by older, less massive stars. There are no prominent spiral arms or strong dust lanes visible, indicative of a relatively quiescent galaxy with a low star formation rate. There are no obvious signs of recent major merger activity or significant tidal disturbances in the main body, although subtle asymmetries cannot be entirely ruled out. The estimated size appears consistent with that of a typical galaxy at its redshift.
