The galaxy exhibits a disk-like morphology, though it is not perfectly symmetrical. There is a slight inclination relative to our line of sight, but not quite edge-on. The central bulge appears to be compact and relatively bright. There is some indication of spiral arm structure, but it appears somewhat disrupted or irregular. The overall color profile suggests the presence of both older stellar populations in the central bulge and younger, bluer stars in the disk. Faint tidal features are apparent extending from the galaxy, particularly towards the lower end, indicating possible gravitational interaction with another galaxy or past merger events. These features are diffuse and less defined. Overall the image is consistent with a spiral or lenticular galaxy undergoing minor interactions.
