This galaxy exhibits a clear spiral structure, characterized by well-defined arms extending from a central region. The arms themselves appear to be moderately tightly wound, displaying a relatively uniform appearance throughout the galaxy. The overall color profile suggests a mix of stellar populations, with a slightly more yellowish hue towards the central regions and a bluer tinge in the outer spiral arms. The galaxy seems to have a weak bar. The central bulge appears to be moderate in size. There is no visually apparent major ongoing merger activity, though there are some disturbances in the shape of the disc, suggesting the possibility of prior interactions or minor disturbances within the galaxy itself.
