The galaxy presents as a somewhat smooth, elongated structure. A dominant central bulge is visible, with a slightly diffused appearance. Faint, extended features may indicate the presence of a disturbed disk, although the image resolution limits a definite classification. There appears to be a possible ongoing merger or interaction with a smaller companion galaxy based on the distortions. The color profile is relatively uniform, suggestive of an older stellar population with comparatively low levels of on-going star formation. The galaxy is a considerable distance away, as evidenced by its redshift, placing it at a significant lookback time.
