The galaxy appears to be a spiral galaxy, likely seen at a fairly high inclination. A central bulge, possibly elliptical in nature, is visible with a yellowish hue. The spiral arms are faint and appear somewhat disrupted or flocculent. They are bluer in color, especially on the left side, suggesting ongoing star formation within these regions. The disk is not perfectly symmetrical, appearing slightly elongated along the axis, which could indicate a mild interaction or disturbance in the past. Evidence suggests the galaxy is forming a moderate amount of stars for its mass.
