The galaxy appears to be a spiral, viewed at a relatively high inclination. The central bulge exhibits a yellow-orange hue, possibly indicative of an older stellar population and a lower rate of ongoing star formation. The outer disk regions show bluer tinges, suggesting the presence of younger, hotter stars. Although the galaxy is mostly smooth, some irregular features and distortions in the disk could indicate gravitational interactions, or perhaps internal processes like star formation that are causing small disturbances. No obvious major mergers or prominent tidal tails are apparent. The galaxy's overall light profile seems fairly uniform, with a smooth transition from the bulge to the outer disk.
