This galaxy exhibits a spiral morphology, albeit somewhat distorted. The central bulge region appears bright and relatively smooth, with a diffuse, blue-shifted emission indicating ongoing star formation. Two apparent spiral arms extend from the core, one more prominent than the other. These arms display a clumpy structure, consistent with HII regions or areas of enhanced star birth. There are signs of potential gravitational disturbance, as the shape is not uniformly circular, and the disk is not perfectly flat. The overall color is a mixture of blue and red, suggesting a combination of younger, hotter stars and an older stellar population. There's some suggestion of tidal interactions, though no clear sign of a distinct merging companion visible in this field. The galaxy's shape is more elongated than circular.
