The galaxy presents a generally elliptical morphology, appearing somewhat smoothed and showing no prominent spiral arm structure. The core region appears to be relatively bright, exhibiting a slightly reddish or yellowish hue, suggestive of an older stellar population. Fainter, bluish regions are observed in the outer parts of the disk, which are indicative of ongoing star formation. There are minor asymmetric features in the disk, but the overall form does not indicate a major ongoing merger. The light distribution suggests it is moderately massive.
