The galaxy presents as a centrally concentrated, luminous object. Its morphology is predominantly smooth, with a high degree of circularity. There is little to no visual evidence of spiral arms or a well-defined disk structure. The light distribution appears to be relatively even, indicating a lack of significant dust lanes or clumpy star formation regions. The galaxy exhibits a slight color gradient, with a somewhat yellower core transitioning to a bluer outer halo or envelope. There is no strong visual indication of major mergers or tidal disturbances, although the presence of minor disturbances cannot be completely ruled out at this resolution.
