The galaxy presents as a largely featureless elliptical morphology. It exhibits a smooth, centrally concentrated light distribution. Its overall color is skewed toward the redder end of the spectrum, which is consistent with an older stellar population and a lower rate of on-going star formation. The galaxy appears to be relatively isolated, without obvious signs of tidal disturbances or major interactions with neighboring galaxies. Its shape is close to round, with only a slight deviation towards an elongated form. No distinct spiral arms, bars, or other disk-like structures are discernible. The galaxy is a regular shape with no major disturbances.
