The galaxy presents as a centrally concentrated object, displaying a roughly elliptical morphology. A smooth luminosity gradient is observed, decreasing radially from a bright, compact core. The core exhibits a yellowish-orange hue, potentially indicative of an older stellar population and/or significant dust extinction. The outer regions of the galaxy are less luminous and appear slightly bluer in color, suggesting the presence of a younger stellar population. No distinct spiral arms or bar features are readily apparent. The overall structure suggests an evolved system with minimal ongoing major mergers or significant tidal disturbances, though a minor disturbance can not be ruled out.
