The galaxy appears to be a spiral galaxy, observed at a slight angle relative to face-on. There is a distinct, though somewhat diffuse, disk structure. Faint spiral arms are visible, emanating from a central bulge. The bulge appears relatively small compared to the overall size of the galaxy. The galaxy's color distribution suggests a presence of both older stellar populations (towards the red end of the spectrum) and younger, star-forming regions (indicated by bluer hues), particularly within the spiral arms. There may be some slight distortion in the disk, possibly indicating minor tidal interactions or internal disturbances. The overall structure does not suggest a major ongoing merger. The galaxy does not appear to be particularly bright, relative to other galaxies in the field.