The galaxy appears to be a luminous, elliptical system, exhibiting a smooth, centrally concentrated morphology. The light profile suggests minimal discernible features such as spiral arms or prominent dust lanes. The core exhibits a bright, yellowish hue, potentially indicating an older stellar population. The isophotes appear largely regular and round, with only a slight deviation from perfect circularity, suggesting a low degree of rotational support. There is no obvious sign of tidal tails or distortions, hinting at a lack of recent major merger activity. A small region to the right of the galaxy shows some slight reddening which could be due to a small region of dust, though the light from this region is dim.
