The galaxy presents as a centrally concentrated, relatively smooth, and luminous object. It appears elliptical in shape, with a high degree of circularity. There is a noticeable color gradient, transitioning from a bright, orange-yellow core to a fainter, greenish halo or outer region. The central bulge is dominant, suggesting an older stellar population. There is little evidence of spiral arms, distinct dust lanes, or active star formation regions. The galaxy appears largely undisturbed, with no obvious signs of ongoing or recent major mergers or tidal interactions. Its overall morphology suggests a well-formed, evolved system, consistent with an early-type galaxy.
