The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall color appears yellowish-orange, suggesting an older stellar population and a relatively low rate of recent star formation. There is no clear evidence of spiral arms or a prominent disk structure. The light distribution gradually fades from the central core outwards, indicating a high degree of radial symmetry. Subtle color variations are visible, with the core appearing more golden and the outer regions exhibiting a slightly redder hue, which could be due to differences in stellar populations or dust content. There is no apparent major ongoing merger or strong tidal disturbance visible within the image, although some subtle irregularities in the outer halo might suggest minor past interactions. The galaxy appears largely quiescent, with little evidence of active star-forming regions.
