The galaxy presents as an elliptical or lenticular type, displaying a centrally concentrated bulge surrounded by a fainter, extended disk. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population. The outer disk appears slightly bluer in color, potentially indicating ongoing star formation. There is a degree of asymmetry visible in the disk, but no obvious signs of major disturbances or mergers. The overall shape is elongated, rather than perfectly circular. The light distribution across the galaxy appears relatively smooth.
