This galaxy presents as a spiral type, viewed at a slight angle from face-on. The central bulge appears moderately prominent and luminous, exhibiting a concentrated brightness. Spiral arms are distinctly present. There is a suggestion of a bar-like structure, although it is not particularly pronounced, which might be characterized as a weak bar. The arms themselves are tightly wound around the bulge, creating a compact appearance. In terms of color, the galaxy exhibits a bluer hue, which potentially indicates recent or ongoing star formation activity. This color is particularly noticeable along the spiral arms. However, the arms exhibit regions with differing luminosity. There are areas with a higher concentration of brighter spots, which could indicate dense regions of star formation or stellar clusters. Overall, the galaxy appears to be a reasonably well-defined spiral galaxy with moderate star formation activity occurring in its spiral arms. There is no conclusive evidence of ongoing major merging activity from the image, although the presence of some asymmetry or tidal features should be considered.
