The galaxy presents a largely smooth morphology, with a concentrated central bulge that exhibits a yellowish hue, suggestive of an older stellar population. The galaxy appears to be primarily elliptical in shape, though there may be a slight disk component contributing to a weak, elongated structure. There is no strong evidence of spiral arms or distinct morphological features. The outer regions fade gradually into the background, indicating a diffuse stellar halo. No significant signs of recent major merger events are observed, although minor disturbances or interactions cannot be ruled out at this resolution. Overall, the galaxy appears to be a relatively evolved system with a dominant spheroidal component.
