The galaxy presents as a relatively smooth and centrally concentrated object. Its morphology appears to be elliptical, with a high degree of rotational symmetry. The galaxy exhibits a radial color gradient, appearing more yellowish-white in its core and gradually transitioning to a redder hue in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy is moderately elongated, suggesting an oblate spheroidal shape. There may be some very minor disturbances in the out regions of the galaxy, possibly due to a past minor merger. There is little to no visible evidence of ongoing star formation within the galaxy.
