The galaxy appears to be an elliptical or lenticular type, exhibiting a relatively smooth and centrally concentrated morphology. The light distribution suggests a moderate degree of ellipticity, not quite spherical but also not highly elongated. The primary color of the galaxy appears to be a yellowish-orange, indicative of an older stellar population with fewer young, hot stars. Fainter bluish-green hues are visible in the outer regions which may indicate the presence of some younger stars, or regions of more recent star formation. There is no clear evidence of spiral arms or a distinct disk structure. There is no apparent strong tidal interaction or merger event, the galaxy's overall form appears relatively undisturbed.
