The galaxy presents as a moderately sized, face-on or nearly face-on system. It displays a central, concentrated region of high luminosity, suggestive of a significant bulge component or active galactic nucleus. Surrounding this central region is a fainter, more diffuse disc. This disc shows some subtle features suggesting the presence of spiral arms. There appears to be some disturbance within the disk. Color gradients are present, with the central region exhibiting bluer hues potentially indicating younger stellar populations, while the outer regions are redder, which might indicate older stellar populations and a higher concentration of dust. Overall, the galaxy exhibits characteristics indicative of a spiral or lenticular type with signs of some type of galactic interaction.
