The object appears to be a spiral galaxy. A prominent central bulge dominates the core region, exhibiting a bright, concentrated luminosity. Spiral arms extend outward from this bulge in a relatively tightly wound configuration. While the central bulge has a noticeable yellow/white tint, the arms are bluer in color. The arms are not perfectly symmetrical, appearing somewhat patchy and showing signs of active star formation regions. Dust lanes can also be seen weaving through the spiral arms. There is little to no evidence of any major interaction with another galaxy, though slight asymmetries in the arm structure suggest the possibility of minor disturbances. The disk is viewed at a noticeable angle.
