The galaxy presents a largely smooth morphology, appearing primarily as an elliptical-type galaxy at a redshift of approximately 0.21. The light distribution is concentrated towards the center, suggesting a prominent bulge. The galaxy exhibits a moderate degree of roundness. There is no obvious spiral arm structure or strong evidence of ongoing mergers or major disturbances. The color profile shows a relatively red hue, possibly indicating an older stellar population and a low ongoing star formation rate.
