The object presents as a spiral galaxy, viewed at a significant inclination. The spiral arms are tightly wound around a prominent central bulge. The bulge appears yellowish, suggestive of an older stellar population. The spiral arms exhibit a bluer hue, indicative of ongoing star formation. Dust lanes appear to be present within the spiral arms, particularly on the near side of the galaxy due to the inclination. The galaxy does not appear to have any major or minor disturbances in its form. It appears to be in relative isolation.
