The galaxy presents an overall smooth morphology, lacking distinct spiral arms or a prominent bar structure. It exhibits a centrally concentrated bulge that appears roughly spherical. The color gradient suggests an older stellar population concentrated in the core, with the bulge displaying a yellowish-orange hue. Moving outwards from the core, the light appears more blue, suggesting the potential presence of younger, hotter stars in the outer regions. The galaxy displays a moderate degree of ellipticity, appearing more oval than perfectly circular. There appears to be no major ongoing merger events, nor any clear signs of significant tidal disturbances in its immediate vicinity.
