The galaxy appears as a somewhat rounded, centrally concentrated object. The light distribution is relatively smooth, indicating a likely elliptical morphology or a spiral galaxy seen face-on with a dominant bulge. There is no obvious spiral arm structure visible. The galaxy exhibits a color gradient, with a slightly redder core, implying an older stellar population, while the outer regions show hints of bluer colors, possibly due to ongoing or recent star formation. There's no obvious indication of any significant tidal disturbances or merger activity in the immediate vicinity, suggesting a relatively isolated system, although minor disturbances cannot be ruled out. The galaxy possesses an estimated mass on the higher end of the scale, with moderate levels of star formation.
