The galaxy presents an overall elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a relatively featureless appearance, suggesting an older stellar population. A subtle colour gradient is observed, with the central bulge appearing slightly redder than the outer regions of the galaxy, possibly indicative of differing stellar population ages and metallicities. There is faint evidence of a disk structure, but it is heavily obscured by the primary spheroid. No clear spiral arms or bar structures are visible. There is very slight distortion in the light distribution, suggesting possible recent or ongoing minor merger activity.
