The galaxy appears as a somewhat symmetrical, centrally concentrated object. It exhibits a smooth, diffuse morphology with no readily discernible spiral arms or bar structure. The color profile suggests a predominantly older stellar population, with a subtle color gradient becoming bluer towards the outer regions, potentially indicating some ongoing, though subdued, star formation. There's no clear evidence of significant dust lanes or prominent star-forming regions within the galaxy, and it presents a generally quiescent appearance. There's only very minor distortion visible within the galaxy. The galaxy is slightly elliptical, but generally rounded.
