The galaxy presents as a slightly inclined, elongated spiral galaxy. The central bulge appears smooth and exhibits a concentrated, diffuse glow of light, suggesting an older stellar population. Faint spiral arms extend outward from the central region; these arms are not sharply defined, but instead show a flocculent structure.

The color distribution across the galaxy indicates a range of stellar populations. The central bulge appears relatively redder. The spiral arms exhibit hints of bluer hues, possibly indicating the presence of younger, hotter stars and ongoing star formation. There are no obvious signs of significant dust lanes or other prominent features within the galaxy's disk. There is some disturbance of the galactic disk that could be related to a minor merger.
