The galaxy presents as a somewhat elliptical, but mostly round, shape, exhibiting a smooth overall structure. A bright central region appears to be present, possibly indicating a galactic bulge or active galactic nucleus. The light distribution suggests a relatively homogeneous stellar population, with a color gradient toward the center. The galaxy displays a blue hue, possibly indicative of active star formation, although it also could simply be a result of the redshift from its location. There are no prominent spiral arms or obvious signs of a recent major merger event visible, but there seems to be minor disturbances with a possible faint tidal feature or asymmetry on one side, suggesting potential interaction with a companion galaxy or past merger.
