The galaxy presents as an elliptical-type system with a smoothly distributed luminosity profile. There is a higher concentration of light towards the galactic center, gradually diminishing outward. The galaxy appears to have a moderate inclination relative to the observer. The object exhibits a yellowish hue indicative of an older stellar population, with little evidence of active star formation. The morphology appears relatively undisturbed, showing no major signs of recent mergers or interactions. There is a slight elongation in its shape but it mostly presents as a rounded system. 
