The galaxy presents a generally smooth, elongated morphology, appearing more cigar-shaped than circular. The light distribution suggests a central concentration of stars or other luminous matter with a relatively smooth radial falloff.  The color gradient indicates a predominantly older stellar population throughout the galaxy, with a hint of more recent star formation activity at the core, which has a slight blueish tint. There does not seem to be any significant ongoing merger activity or strong tidal disturbances, although some minor asymmetry is apparent. The overall structure hints at a galaxy in the process of transitioning to an elliptical morphology.
