The galaxy presents as a spiral with tightly wound arms. A distinct, yellowish central bulge is evident, appearing relatively small in proportion to the overall galactic disk. The spiral arms are well-defined, exhibiting a clumpy structure indicative of ongoing star formation. The galaxy displays a blueish hue in the arms, suggesting the presence of young, hot stars. There is no strong evidence of a bar structure. Overall, the galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal distortions.