The galaxy presents as a relatively smooth object, exhibiting a central bulge that gradually diffuses into a less structured disk. The galaxy possesses a yellowish-white hue centrally, suggestive of an older stellar population. The disk shows hints of bluer regions, potentially indicative of ongoing, though possibly limited, star formation. There appears to be no strong evidence of major disturbances or a recent merger event in this image, though minor tidal features cannot be entirely ruled out given the image resolution. The overall morphology appears to be close to round, showing only minimal elongation.
