The galaxy presents as a relatively smooth, elliptical-like structure with a slight elongation along its major axis. A bright central bulge is visible, exhibiting a more concentrated light profile. The outer regions of the galaxy appear less defined, fading gradually into the background sky. There's a subtle color gradient, with a slightly bluer hue in the outer disk, suggestive of some ongoing star formation, transitioning toward redder colors in the central bulge, potentially indicating an older stellar population. There appear to be no significant signs of spiral arm structures or major disturbances indicative of recent merger events. Small disturbances cannot be ruled out. Overall, the galaxy appears as a moderately massive system at intermediate redshift.
