The galaxy appears to be a relatively smooth, centrally concentrated system, likely an elliptical or lenticular galaxy, observed at redshift. The light profile is quite compact. There is a slight extension of the main body, but no distinct spiral arm structures are discernible. The central region exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy display a faint, bluish tint, which might indicate ongoing, although subdued, star formation. There is no evidence of any significant merger activity or major morphological disturbances, though it is possible that minor interactions have occurred in the past given the slight irregularity. The galaxy's overall structure is dominated by its spheroidal component.
