This galaxy exhibits a generally smooth morphology with a high degree of central concentration. The light profile appears relatively featureless, lacking prominent spiral arms or a distinct disk structure. The core of the galaxy displays a yellowish hue, which suggests the presence of an older stellar population. The outskirts of the galaxy show a subtle color gradient, transitioning to a slightly bluer tint, which is characteristic of some younger stars mixed in with the older population. There is no evidence of major ongoing mergers or significant tidal disturbances, although a few very slight irregularities might suggest minor interactions or past merger events. The overall shape appears close to circular.
