The galaxy appears to be a spiral type, presenting a somewhat tilted orientation relative to our line of sight. There is evidence of spiral arm structure, though these features exhibit a degree of flocculence. The arms are not sharply defined but instead appear somewhat patchy. A central bulge is visible; moderate in size and luminosity. The arms exhibit a relatively tight winding pattern, suggesting a considerable degree of shear. The galaxy's overall color suggests a population that contains both older, redder stars and younger, bluer stars, concentrated within the arm features. There is no obvious indication of a major ongoing merger event, though some minor disturbances in the outer regions cannot be ruled out given the irregular arm structure. Overall, the morphology suggests a spiral galaxy that has likely experienced some gravitational interactions, evidenced by the loose spiral arm structure.
