The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, appearing mostly round, with a minor elongation. The central region displays a yellowish hue, possibly indicating an older stellar population. Moving outward from the center, the color transitions to a bluish halo, suggesting the presence of younger, hotter stars and perhaps ongoing star formation in the outer regions. There are no obvious signs of major disturbances or ongoing mergers, although subtle asymmetries might indicate minor interactions or internal dynamics. Overall, the galaxy presents as a fairly well-ordered and evolved system with some residual star-forming activity.
