The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, featureless morphology. The light profile suggests a centrally concentrated bulge that constitutes the galaxy's primary structure. The core displays a bright, yellowish-orange hue, which may suggest an older stellar population with relatively low star formation. Moving outward from the center, the color transitions to a bluer tone, with a hint of a disk-like structure visible. There may be the presence of weak spiral arms or a diffuse, extended disk but these features are not distinct. The overall shape deviates slightly from perfectly round, showing a hint of elongation. There is no clear evidence of major mergers or significant tidal disturbances.
