The galaxy presents as a spiral type, characterized by a distinct central bulge surrounded by a relatively well-defined disk. The spiral arms exhibit a two-armed structure, loosely wound around the central bulge. The arms show a clumpy, textured appearance indicative of ongoing star formation regions. The central bulge appears moderately luminous and exhibits a yellow-white color, suggesting an older stellar population compared to the bluer arms. The overall luminosity indicates a galaxy with an intermediate stellar mass. There appears to be no significant bar structure. The disk shows no significant edge-on inclination. There is little to no indication of a major merger event. The galaxy shows a relatively undisturbed morphology, with some potential for minor disturbances.
