The galaxy presents a primarily smooth and rounded morphology. Its core exhibits a concentrated, bright luminosity, indicative of a significant stellar population density. The outer regions appear less defined, exhibiting a gradual decrease in brightness as the distance from the center increases. The galaxy displays a slight ellipticity. There is evidence of possible tidal disturbances or faint plumes that may suggest past or ongoing minor interaction. Overall, the galaxy appears to be a relatively evolved system with a dominant bulge component.
