The galaxy presents as a spiral type, with a moderately inclined disk relative to the observer's line of sight. The central bulge appears prominent and exhibits a yellowish hue, indicating a likely older stellar population. Spiral arms are readily apparent, tracing a well-defined pattern extending outward from the bulge, with hints of numerous and tightly wound spiral arms. The arms display a bluish tinge, suggesting the presence of younger, hotter stars and ongoing star formation. Patches of red are sparsely distributed within the arms. Overall morphology suggests a relatively undisturbed galaxy, lacking strong evidence of recent major mergers or interactions.
