The galaxy presents as a moderately luminous object at a redshift of approximately 0.17. It exhibits a somewhat elliptical morphology, appearing elongated along its major axis. The galaxy's light distribution suggests a relatively smooth profile, with the majority of its luminosity concentrated towards the central region. The color gradient reveals a subtle trend, with the core region displaying a slightly yellower hue compared to the outer regions. A small percentage of observers have reported the presence of a merger or disturbance. I conclude that this galaxy is likely a relatively old, massive system that has experienced minor interaction or is currently undergoing it. The star formation rate is comparatively low, with an estimated mass of greater than 10^10 solar masses. 
