The galaxy presents as a likely spiral, though its morphology is somewhat disturbed. There is a prominent central bulge surrounded by a fainter disk. Indications of spiral arms are subtle, perhaps due to the relatively high redshift, though some structural asymmetry is apparent. The redder color, particularly concentrated within the bulge, suggests an older stellar population. The integrated light indicates that the galaxy exhibits a blue component, particularly in what appears to be segments of the spiral arms. Some level of star formation is likely occurring. Indications of a past or ongoing minor merger event are present, possibly contributing to its irregular appearance. The size of the galaxy appears to be consistent with a galaxy of significant mass.
