The galaxy appears as an elongated, elliptical shape with a smooth, diffuse structure. The central region exhibits a higher concentration of light, appearing brighter and slightly redder in color, suggesting an older stellar population. Fainter, more diffuse light extends outwards from the core, forming a halo. There is a slight color gradient, with the outer regions appearing slightly bluer, potentially indicating younger stars. The overall morphology appears undisturbed with no visual signs of spiral arms or a bar. The galaxy is likely relatively massive, with a low star formation rate. There is no evidence of a major merger or significant tidal disturbances.
