The galaxy presents an overall elliptical morphology, with a smooth and diffuse light distribution. The central region exhibits a bright, concentrated core that gradually fades into the outer regions. The galaxy does not display any prominent spiral arms or a well-defined disk structure. There is a subtle suggestion of some disturbed features in the outer regions, with one side appearing slightly more extended. The color profile seems relatively uniform with a hint of bluer tones near the core that could suggest the possibility of some ongoing star formation activity. There appear to be no other galaxies interacting with this galaxy, but it could have had some interactions in the past, creating the observed disturbances.
