The galaxy presents a generally smooth and rounded morphology. There is a slight deviation from perfect sphericity, leaning towards an intermediate elliptical shape. The galaxy's light profile appears centrally concentrated with a gradual decrease in intensity outwards. No distinct spiral arms or bar structures are discernible. The overall color is reddish, suggesting an older stellar population and a relatively low rate of on-going star formation. There might be a possible merging event visible. The primary galaxy shape is disturbed, with slight asymmetry in its light distribution.
