The galaxy presents as a relatively smooth, disk-dominated system. The central bulge appears prominent and exhibits a yellowish-white hue, suggesting an older stellar population. The disk is observed nearly edge-on, with subtle color variations along its extent. The overall color profile of the disk indicates a mix of stellar populations, including some regions that could be indicative of ongoing or recent star formation. There is no strong evidence of a major ongoing merger, but the morphology suggests minor disturbances may be present. Based on visual inspection, the galaxy appears moderately massive.
