The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light distribution. There is a noticeable radial color gradient, with the core displaying a yellowish-white hue, transitioning to a redder color in the outer regions. The isophotes are generally smooth and elliptical, with the ellipticity suggesting a deviation from a perfect sphere. No distinct spiral arms or dust lanes are visible. There is no evidence of ongoing major mergers, although a possible minor disturbance is implied by a slight asymmetry in the outer halo. Based on the observed color and smooth morphology, the stellar population likely consists predominantly of older, evolved stars, suggesting relatively low levels of current star formation. The overall structure suggests a massive system.
