This galaxy presents as a spiral galaxy, viewed at a moderately inclined angle. Spiral arms are discernible, though not tightly wound. They appear somewhat patchy and asymmetric, suggesting ongoing or recent star formation within the disk. There is a significant central bulge, appearing yellowish-white, which could indicate a substantial population of older stars. The disk component exhibits a bluer color, consistent with younger stellar populations and star-forming regions. Overall, the galaxy appears relatively well-defined and moderately bright, with a hint of internal structure within the spiral arms. There is no strong indication of tidal disturbances, but subtle distortions within the outer disk are possible.
