The galaxy presents a spiral morphology. The spiral arms are tightly wound and somewhat indistinct. The central bulge appears moderate in size, exhibiting a concentrated luminosity. Evidence of a bar structure is not strongly apparent, although subtle asymmetries could suggest a weak bar feature. The disk is not viewed edge-on. There is some visual indication of star formation within the disk, as evidenced by slightly bluer regions within the spiral arms, even though the arms themselves are indistinct. There is no clear evidence of a major merger or strong tidal disturbance in this image, but there may be very minor disturbance. The galaxy is oriented approximately horizontally in the image frame.
