The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting a high degree of roundness with minimal deviation from a circular form. There is a noticeable color gradient, transitioning from a yellowish-white core region to a bluer outer halo. No distinct spiral arm structure or prominent dust lanes are discernible. Indications of any recent major merger events or significant tidal disturbances are absent, with a slight possibly asymmetrical bulge. The overall morphology suggests a galaxy that has undergone significant spheroid formation. Star formation appears low, as it seems to be dominated by an older stellar population.
