The galaxy exhibits a somewhat lenticular morphology, appearing as a flattened disk-like structure oriented approximately edge-on to our line of sight. A central bulge is visible, appearing relatively smooth and concentrated. The disk component shows hints of spiral structure, characterized by faint, diffuse arms extending from the central region. There are subtle color variations across the galaxy, with a bluer hue in the outer disk, and a warmer redder hue in the central bulge, possibly indicative of ongoing star formation in the arms. A dust lane, although faint, appears present along the equatorial plane, obscuring light from the far side of the disk. No signs of a major merger are readily apparent, although minor disturbances or tidal features cannot be ruled out with this image resolution.
