The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology, suggesting an elliptical or lenticular classification. The light profile appears circularly symmetric with a slight elongation. A dominant, yellow-orange hue characterizes the galaxy's core, potentially indicating an older stellar population. Fainter, diffuse, bluish extensions are seen along the outer fringes, perhaps indicative of more recent star formation or tidal features, however the overall smoothness is most prominent. The surrounding light distribution appears relatively undisturbed, with no obvious signs of major mergers or strong tidal interactions with nearby galaxies.
