The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Color gradients are observed, with a yellow-orange hue dominating the central region, suggesting an older stellar population. A slight bluish tinge is visible in the outer regions, potentially indicating the presence of younger, hotter stars, although this feature is less pronounced. There is no evidence of spiral arms or a distinct disk structure. The overall form suggests a galaxy that has largely ceased active star formation. Interactions with neighboring galaxies are not immediately apparent, as the overall form is consistent with a relatively undisturbed galaxy. The galaxy's apparent roundness reinforces this impression.
