The galaxy presents a spiral structure, exhibiting a relatively high degree of organized rotational symmetry. The spiral arms are somewhat flocculent, with a notable presence of bright star-forming regions interspersed along their lengths. These regions appear more prominent in bluer wavelengths, suggesting ongoing active star formation.

A central bulge is visible, with an intermediate size in comparison to the overall galaxy. The bulge displays a smoother texture and a more reddish hue relative to the spiral arms, indicative of an older stellar population.

There is a possible indication of a bar feature bisecting the galaxy. The galaxy does not appear to be undergoing a major merging event, though there may be some minor morphological disturbances. Overall, the galaxy appears to be a relatively normal spiral galaxy.
