The galaxy presents as a relatively smooth, elliptical-like object, exhibiting a centrally concentrated brightness profile. The core region displays a bright, almost unresolved nucleus, suggesting a significant concentration of stars. The overall color of the galaxy appears to be in the yellow-red range, potentially indicative of an older stellar population, with a minor contribution of light in the blue range. No distinct spiral arm structures are discernible. The absence of strong dust lanes supports the interpretation of a well-mixed stellar population. The object's shape is approximately elliptical, with only a slight deviation from a perfectly round morphology. There appears to be no major ongoing merger activity or significant tidal disturbances in its immediate vicinity. 
