The galaxy appears to be a relatively smooth, elliptical-like structure, likely at an intermediate redshift. It exhibits a notable central concentration of light, suggesting a prominent bulge. There is a slight elongation that prevents it from being perfectly circular, with a suggestion of a disk component. The galaxy displays a reddish-yellow color, indicating an older stellar population and relatively low levels of ongoing star formation. Some evidence of minor disturbance is noted through potential asymmetrical morphology, possibly due to a past minor interaction or merger event. The galaxy is relatively compact and possesses a moderate absolute magnitude.
