This galaxy presents as a spiral type, viewed at a moderate angle from edge-on. A prominent disk structure is apparent, though it is not perfectly symmetrical. Spiral arms are clearly visible, appearing tightly wound near the central bulge, then loosening as they extend outward. Two distinct spiral arms are particularly noticeable. A bar structure traverses the central region, with a moderate strength.

The central bulge appears moderately sized. The overall color profile suggests ongoing star formation, particularly within the spiral arms, with some regions exhibiting bluer hues. The galaxy appears relatively isolated, without signs of major mergers or significant tidal disturbances.
