This galaxy presents as a spiral type, with discernible, loosely wound spiral arms extending from a central bulge. The arms exhibit a somewhat flocculent structure, with a non-uniform distribution of luminosity. The central bulge appears moderately prominent and elongated. There is evidence of a bar-like feature spanning across the center of the galaxy, but it is not distinctly defined. The color profile suggests active star formation within the spiral arms. There also appears to be some disruption occuring in the arm structure, which may indicate a merger event. 