The galaxy presents as a somewhat elliptical, disk-dominated system. It exhibits a smooth light distribution with a bright central bulge, suggesting a significant concentration of older stellar populations toward the galactic nucleus. Fainter, diffuse light extends outwards from the bulge in a flattened structure, likely representing the galactic disk. There is little evidence of defined spiral arms. The colour gradient transitions from a yellow-white core to a fainter, slightly bluer outer disk. The overall smooth texture and lack of prominent features suggest a relatively quiescent galaxy.
