The galaxy presents a predominantly smooth morphology, with a bright central bulge. Its overall color appears to be on the redder side, suggesting an older stellar population. The primary structure seems relatively undisturbed, with no obvious signs of recent major mergers. However, there is a suggestion of a smaller galaxy nearby that might indicate a potential interaction or past merger event. The isophotes of the main galaxy appear generally elliptical, but with some degree of irregularity.
