The galaxy appears to be a relatively small, elongated spiral galaxy, presenting itself nearly edge-on to our line of sight. It is characterized by a central bulge that seems moderately prominent. Faint traces of a disk are discernible, though their detailed structure is obscured by the viewing angle. The spiral arms are not clearly resolved, but their presence is suggested by slight color variations and subtle undulations in the galaxy's overall form. There is no obvious evidence of a major ongoing merger, although a subtle disturbance or minor interaction cannot be completely ruled out. Overall, the galaxy displays a morphology consistent with a late-type spiral, though a definitive classification is challenging due to its orientation.
