The galaxy presents as a relatively symmetrical, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish, suggestive of an older stellar population. The disk component is less prominent, displaying a bluer hue that could indicate more recent star formation. There are some irregular features in the arms, potentially indicating minor disturbances, but no clear signs of ongoing major mergers are detected. The overall morphology suggests a system transitioning from a more active star-forming phase to a quiescent state. The estimated size is likely a few kiloparsecs across.
