The galaxy presents as a spiral type with a prominent central bulge and distinct, well-defined spiral arms. These arms exhibit a somewhat flocculent structure. There appears to be a moderate amount of ongoing star formation activity within the arms, indicated by regions of bluer color, although they are not very clumpy. The bulge dominates the central region, with a strong concentration of light. There is no obvious bar structure visible. The galaxy appears relatively undisturbed. Its estimated effective radius is approximately 5 kpc.
