The galaxy presents as an elliptical form, exhibiting a smooth, featureless morphology across its visible extent. The light profile appears centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. The overall color is slightly redder in the central bulge, suggesting an older stellar population. A subtle, faint blue halo is seen extending from the mid plane of the bulge, likely indicating recent or ongoing star formation in the outer regions. The shape of the galaxy appears somewhere between an ellipse and a flattened football, suggesting it is rotating. There is no apparent signs of tidal disruption or interaction with any other system.
