The galaxy appears to be a relatively smooth, elliptical-type galaxy, though a subtle disk component cannot be ruled out. It exhibits a generally round morphology, showing a slight degree of elongation. Color gradients are present, with a yellowish-white core that transitions to a redder outer halo, suggesting an older stellar population is dominant. There is no distinct dust lane or spiral arm structure visible in the image. Faint irregularities are visible, possibly indicating a minor interaction or disturbance with another galaxy.
