The galaxy presents as a moderately luminous spiral, characterized by a central bulge and a discernible disk structure. The bulge appears relatively smooth and concentrated, exhibiting a yellowish hue, suggesting a population of older stars. A distinct spiral arm extends from one side of the disk, displaying a clumpy morphology with regions of active star formation evident in its bluer color. The opposite side of the disk is less defined. There are no major disturbances visible in the galaxy's morphology, but the slightly warped appearance of the disk hints at the possibility of minor gravitational interactions or internal dynamic processes. Overall, the galaxy appears to be in a relatively quiescent state of star formation.
