The galaxy presents as a spiral morphology, viewed at a slight angle relative to face-on. Two well-defined spiral arms are visible, exhibiting a tightly wound structure that emanates from a moderately sized central bulge. The disk of the galaxy appears to be the dominant feature, presenting a noticeable presence. There is no indication of a substantial bar structure, but a weak bar may be present. The overall structure of the galaxy shows no major signs of significant disturbance from recent mergers or interactions, although a minor disturbance cannot be ruled out. The spiral arms exhibit a consistent blue color, suggesting the presence of ongoing star formation. The central bulge appears more yellowish-red, indicative of an older stellar population.
