The galaxy presents a moderately bright, well-defined elliptical morphology. Its color appears somewhat redder overall, suggesting an older stellar population with suppressed recent star formation. There is a slight elongation to the shape, indicative of a mild deviation from perfect sphericity. The galaxy core exhibits a smooth, concentrated light distribution. There is no visual evidence of prominent spiral arms or dust lanes. Indications suggest little to no ongoing major merger activity or significant tidal disturbances. The galaxy is relatively compact.
