The galaxy appears to be an elliptical type, exhibiting a smooth, symmetrical morphology. It has a noticeable central bulge that is bright and concentrated. The galaxy displays a reddish hue overall, suggesting an older stellar population with lower ongoing star formation. Its shape is elongated, deviating from a perfect sphere and showing an axial ratio of approximately 0.75. There is no evidence of spiral arms or a prominent disk structure. The light distribution falls off gradually from the bright core outwards, indicating a high Sersic index.
