The galaxy appears as a relatively smooth, elliptical-shaped structure with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting a population of older stars. There is little evidence of spiral arms or significant dust lanes, indicating a lack of ongoing, significant star formation. The morphology seems to be largely undisturbed, with no major signs of tidal interactions or recent mergers, although there may be minor disturbances in the outer regions. The galaxy's light profile seems to be centrally concentrated with a gradual falloff in surface brightness away from the core.
