The galaxy presents as a dominant, elliptical-like structure. Its light profile exhibits a smooth, centrally concentrated morphology, with a noticeable color gradient. The core appears to be a bright, golden hue, suggesting a concentration of older stellar populations. This color gradually fades towards the outer regions, exhibiting a more reddish-yellow tint. The overall form is somewhat elongated, though not dramatically so. There is no clear evidence of spiral arms or significant dust lanes visible in this image. The galaxy appears relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers in the immediate vicinity. The smooth features, coupled with the color profile, indicate it may be a mature system. The morphology is consistent with an elliptical galaxy which is quiescent with minimal star formation.
