The galaxy presents an overall elliptical morphology, with a dominant spheroidal component. The central region exhibits a high concentration of light, appearing bright and yellowish, suggesting an older stellar population. Moving outward from the core, the galaxy's luminosity gradually decreases, fading into a less defined halo. There is some distortion in the outer edges of the halo that suggest tidal disturbances or potential ongoing mergers. The shape is neither perfectly round, nor highly elongated. Though somewhat blurry in this image, the galaxy exhibits a relatively smooth appearance. There appears to be no distinct spiral arm structure, and the dust lanes are not apparent.
