The galaxy presents as a smooth, rounded object with a concentrated central bulge. There is no clear evidence of a disk structure or spiral arms. The color profile suggests an older stellar population with a yellowish hue dominating the central region, transitioning to slightly bluer colors toward the outer edges, though these are still subdued. There are no obvious signs of recent or ongoing major mergers or significant tidal disturbances in the immediate vicinity. The galaxy appears relatively isolated and undisturbed.
