The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. It exhibits a well-defined disk structure with two prominent spiral arms that wind moderately tightly around a central bulge. The central bulge appears relatively moderate in size. A bar-like structure seems to traverse through the galactic center, though the evidence of the bar is faint, it could be a weak bar. The color distribution shows a bluer hue in the spiral arms suggesting ongoing star formation in these regions, while the central bulge appears more yellow/red, possibly indicating a population of older stars. The image does not show any significant signs of recent or ongoing major merging activity, though there might be a minor irregularity in one of the arms.
