The galaxy presents as a relatively smooth, centrally concentrated object. It is more elongated than circular, appearing somewhat elliptical in shape. The color profile is dominated by warmer tones, suggesting an older stellar population, though there are hints of bluer regions, indicative of more recent star formation, within the galaxy. There is no evidence of a significant, ongoing merger, although there is a suggestion of minor disturbances to the outer structure of the galaxy. The galaxy's overall structure is relatively undisturbed and mostly smooth. The estimated size, given its redshift, suggests that this is a galaxy of moderate size.