The observed galaxy presents as a barred spiral system, although the spiral structure is not particularly well-defined. The galaxy possesses a prominent central bulge, which appears moderately large and exhibits a yellowish hue, indicative of an older stellar population. The bar structure is moderately pronounced. The disk component of the galaxy shows some evidence of spiral arms, although they are somewhat flocculent and not tightly wound. Overall, the galaxy appears to be undergoing a relatively low rate of star formation. There are no major signs of ongoing merger activity.
