The observed galaxy presents as a spiral structure with a relatively prominent central bulge. The spiral arms are not tightly wound; instead, they appear more open and loosely defined, exhibiting a somewhat patchy distribution of light. There is some indication of clumpy star-forming regions within the arms, though these are not exceptionally bright or distinct. The disk of the galaxy appears relatively face-on, allowing for a good view of the spiral structure. The overall color is slightly bluer in the disk and arms, suggesting ongoing star formation, compared to the yellowish hue of the central bulge, which may be indicative of an older stellar population. There is no obvious, large-scale disturbance suggesting a major ongoing merger event, though subtle asymmetries cannot be ruled out.
