The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The central region exhibits a yellowish-white hue, suggestive of an older stellar population. Surrounding the core is a faint, diffuse blueish halo, indicative of some ongoing, albeit low-level, star formation. There is a slight elongation to the galaxy’s shape, but no clear evidence of spiral arms or significant disk features. No major disturbances or merger activity are apparent. The galaxy appears largely isolated and undisturbed.