The galaxy appears to be a relatively smooth, elliptical galaxy, likely at an intermediate redshift. It has a generally round morphology with a high degree of central concentration, suggesting an older stellar population. There is little to no evidence of spiral arms or a prominent disk structure. The light profile is smooth and lacks significant substructure, which further reinforces the impression of a spheroid-dominated system. There are no obvious signs of on-going mergers or significant tidal disturbances. Based on its color, the galaxy likely has a low star-formation rate.
