The galaxy presents as a spiral galaxy with a prominent, although not overwhelmingly dominant, central bulge. The disk component appears to be the dominant feature, exhibiting a relatively high inclination, presenting an elliptical appearance.

Spiral arms are observed, with at least two major arms discernible, though the structure is somewhat flocculent. Star formation is evident within the spiral arms, indicated by a bluer color. There are regions with more concentrated star forming activity, and the arm structure has areas of higher density interspersed with less dense regions. The bulge itself appears smoother and yellower in color, consistent with an older stellar population. A hint of a bar may be present, though it is not sharply defined. There are no signs of major mergers or tidal disturbances.
