The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, displaying a generally rounded shape but with hints of a disk structure. The galaxy exhibits a dominant central bulge, characterized by a bright, almost stellar nucleus, surrounded by a fainter, more diffuse halo. There is no obvious spiral arm structure. The light distribution suggests a higher concentration of older stellar populations and diminished star formation activity. There are no obvious signs of on-going or recent major merger events in the core of this galaxy.

