The galaxy presents as an elliptical-like structure, elongated along its major axis. It exhibits a relatively smooth, diffuse morphology with a high degree of central concentration. The light distribution suggests a dominant bulge component, with a gradual decrease in surface brightness moving outwards. A slight blue hue appears towards the extremities of the galaxy. No distinct spiral arms or prominent dust lanes are discernible within the observed band. The galaxy shows possible signs of minor tidal disturbances or distortions in its outer regions. The overall appearance is consistent with a relatively evolved system, with intermediate star formation activity.
