The galaxy presents as a spiral structure, exhibiting a moderate bulge component. Faint spiral arms are visible, winding loosely around the central bulge. The color profile suggests a mix of stellar populations, with the bulge exhibiting a yellowish hue, possibly indicating older stars, while bluer tinges in the spiral arms could indicate more recent star formation. There may be ongoing gravitational interactions or disturbances with the galaxy, but they appear minor in nature. There appears to be 2 main spiral arms. The galaxy does not appear to be edge-on.