The galaxy presents as a spiral type, with a clearly defined, though somewhat diffuse, disk structure. Spiral arms are evident and appear tightly wound, tracing an almost circular pattern around the galactic center. Two arms are prominently visible. The central bulge is moderately sized and exhibits a yellowish hue, suggesting an older stellar population. The disk shows a bluer color, indicative of ongoing star formation. There appears to be no significant bar structure. No major merger events or tidal disturbances are apparent, although the galaxy appears to have minor irregularities in the arms. Overall, the galaxy exhibits a relatively undisturbed morphology.
