The galaxy presents as a smooth, elongated structure, consistent with an elliptical morphology viewed from a significant angle. The central region exhibits a yellowish hue, suggesting a population of older stars, potentially indicative of a more evolved stellar population with lower rates of current star formation. Moving outwards from the central bulge, the color transitions to a bluer tint. This suggests the presence of younger, hotter stars possibly arranged in a disk-like structure, although this is not distinctly resolved in the image. There are no obvious signs of significant tidal disturbances or major mergers in its recent history. The lack of distinct spiral arms or prominent dust lanes further supports the classification of an elliptical or lenticular galaxy.
