This galaxy presents as an elliptical structure with a smooth, featureless appearance. The core exhibits a concentrated yellowish hue, suggesting an older stellar population is dominant in the central region. Moving outward from the core, the color shifts toward a bluer tone, implying the presence of younger, hotter stars. However, the overall impression is that of an evolved galaxy lacking significant active star formation regions. The galaxy is oblong in shape, appearing more like a flattened spheroid than a perfect circle, with no obvious signs of spiral arms or a prominent disk. There are no visual indications of ongoing major mergers or significant tidal disturbances. The lack of dust lanes or patchy structures further supports the assessment of a relatively quiescent and well-mixed system.
