The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Spiral arms are present but somewhat tightly wound, appearing numerous and difficult to individually resolve. The central bulge is moderately prominent, with a yellowish hue suggesting an older stellar population. A bar structure appears present, extending across a notable fraction of the galaxy's diameter. Star formation appears to be present within the spiral arms, indicated by the bluish tint. There is no obvious signs of major mergers or significant tidal distortions of the galaxy's morphology.