The galaxy presents as a single, relatively compact object with an apparent smooth morphology. The color distribution suggests an elliptical or lenticular classification. A dominant yellowish hue is observed in the central region, possibly indicating a population of older stars and a lower rate of star formation. Fainter, reddish tinges may be present in the outer regions, which could represent subtle dust lanes or regions of weak star formation. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal features. The object's radial profile appears to gradually decrease outwards from its center. 
