The galaxy appears to be a spiral galaxy, seen edge-on from our line of sight. A prominent central bulge is visible, characterized by a concentrated luminosity profile. The outer disk is relatively faint and elongated. Some evidence of dust lanes are present within the disk. There is no visible indication of a strong ongoing merger. The bulge appears to be mostly of a round structure. The galaxy exhibits an overall reddish hue, particularly within the bulge. This would lead one to believe there are older stars present.
