The galaxy presents a generally smooth morphology, appearing as a single object with a centrally concentrated luminosity profile. Its shape is somewhat elliptical, appearing slightly elongated rather than perfectly circular. There is a hint of possible tidal interaction, with a faint extension visible. The galaxy exhibits a color gradient, appearing bluer in the center and redder toward its outer regions. Given its redshift, it appears to be at an intermediate distance. The integrated light suggests a population of intermediate to old stars, with ongoing, relatively low levels of star formation. The lack of defined spiral arms or a prominent disk suggests it is an early type galaxy. There is evidence of some disturbances, but it is likely not undergoing a major merger. 
