The galaxy presents as an elongated, cigar-shaped structure. Its light distribution appears relatively smooth, with a concentrated central bulge. The color gradient suggests a higher concentration of older stars or dust within the central region, giving it a reddish-yellow hue, with fainter blue regions on the peripheries. There is no strong evidence of spiral arm structure or significant disk features. Faint traces of disruption are visible on the bottom side, close to the galaxy. Overall, the galaxy appears to be a lenticular or elliptical galaxy at an intermediate redshift.
