The observed galaxy presents as a spiral type, viewed at a moderate inclination, making it appear somewhat elongated. A prominent central bar structure is visible, oriented approximately horizontally across the galaxy's core. Diffuse spiral arms emerge from the ends of the bar, displaying a somewhat flocculent morphology. These arms exhibit a slightly clumpy structure, suggestive of ongoing star formation regions. The central bulge appears relatively small and indistinct, with a yellowish hue that indicates an older stellar population. The overall color of the disk is a mix of blue and green, implying a blend of younger and older stars. There is no obvious evidence of a major ongoing merger, but the disk structure is not entirely regular, suggesting the possibility of minor interactions or internal disturbances.
