The galaxy presents a flattened, disk-like structure seen at a moderately inclined angle. Its central region exhibits a brighter, concentrated luminosity, suggesting the presence of a galactic bulge. The surrounding disk appears less structured, with a somewhat smooth texture and fainter luminosity extending outwards. The colour distribution indicates a central region with a yellower hue, while the outer disk shows a bluer colour. The overall morphology suggests that the galaxy is likely a spiral galaxy with a pseudo bulge and no distinct spiral arm structure, or an elliptical galaxy. There is some indication of minor disturbances or asymmetry in the outer regions of the disk, possibly due to a minor tidal interaction.
