The galaxy presents as a spiral galaxy, viewed at an oblique angle. The morphology is dominated by its spiral arms. There is a prominent bulge in the center, though its color is not very distinct from the arms. The spiral arms are well-defined and appear somewhat flocculent, exhibiting a winding pattern with areas of both tightly wound and more loosely wound regions. Two spiral arms are visible.

The galaxy exhibits a range of colors across its structure. The central bulge displays a yellowish-white hue, possibly indicating a population of older stars. The spiral arms show a bluer tint, which could indicate the presence of younger, hotter stars and ongoing star formation. There are also areas of reddish coloration, which might represent regions of dust obscuration or older stellar populations. The overall impression is that the galaxy is in a relatively late stage of development, exhibiting both ongoing star formation and older stellar populations. The galaxy also has some signs of disturbance, and its shape is slightly irregular, hinting at a possible interaction or merger event in its history.
