The galaxy presents as a relatively smooth, centrally concentrated elliptical or lenticular structure. It exhibits a yellowish-white hue, suggesting an older stellar population with a diminished rate of ongoing star formation. The galaxy displays a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. No prominent spiral arms or distinct disk-like features are discernible. There is a faint central concentration of light, possibly indicative of a galactic nucleus. The overall morphology suggests a galaxy in a relatively quiescent state, with no obvious signs of major mergers or tidal disturbances. The galaxy shows intermediate brightness, with its color index suggesting the presence of evolved stars.
