The galaxy appears to be a spiral galaxy, observed at a near face-on orientation. Two well-defined spiral arms are visible, winding moderately tightly around a central bulge. The bulge is not particularly dominant, appearing relatively small compared to the overall disk size. A bar structure is present, but it is not particularly strong, and is subtle. There are no signs of any major mergers or significant tidal disturbances, although the galaxy is not completely undisturbed, perhaps due to the presence of a satellite galaxy or minor interaction. The arms show some blue tint, indicating active star formation. The color appears brighter in the r-band relative to the g and z bands.
