The galaxy appears to be a relatively bright, early-type galaxy at a significant cosmological distance. The object exhibits a generally smooth morphology with a high degree of central concentration. A faint, extended halo surrounds the central region. There is no apparent disk structure or spiral arms. The galaxy is generally round in shape with a slight elongation. No major merger events are readily apparent, although the object does exhibit some minor disturbances. The galaxy presents with a reddish hue. This coloration suggests a relatively old stellar population with ongoing star formation.
