The galaxy presents as a spiral galaxy with a moderately sized bulge. The bulge appears yellowish, suggesting an older stellar population. The disk exhibits flocculent spiral arms, though they are not sharply defined, and likely tightly wound. The galaxy is not viewed perfectly edge-on, nor perfectly face-on, presenting at a slight incline. There appears to be a bar structure running through the galaxy, extending beyond the bulge. There is no indication of a major merger. The galaxy exhibits characteristics of a relatively high mass, with the potential of moderate star formation.
