The galaxy appears as a single, centrally concentrated object with a relatively smooth, though slightly irregular, morphology. Its light profile is dominated by a redder central core that gradually fades into a diffuse halo. The object exhibits an overall elliptical appearance, although some subtle deviations from perfect ellipticity are observable. There's a hint of a slight extension, possibly suggestive of tidal interactions or a minor merger event. No distinct spiral arm structures are visible, and the galaxy lacks significant dust lanes or regions of active star formation in this imaging.
