The galaxy presents as a somewhat smooth, elliptical or lenticular structure. It exhibits a noticeable elongation, approximately in a cigar shape. The central region of the galaxy appears brighter and more concentrated, suggesting a bulge. The color profile transitions from a yellowish core to a slightly bluer periphery. There is no clear evidence of spiral arms or distinct disk features. No signs of major disturbances or ongoing mergers are immediately apparent, though a minor interaction cannot be ruled out.
