The galaxy presents as a relatively smooth, elliptical-like structure, appearing somewhat flattened but lacking distinct spiral arms or a prominent disk. The central bulge is luminous, exhibiting a yellowish-white color, suggestive of an older stellar population. The galaxy exhibits a diffuse halo with decreasing luminosity at larger radii. There appears to be little evidence of active star formation regions, with a relatively uniform color distribution. No clear signs of major merging or tidal disturbances are readily apparent. The overall morphology suggests a relatively evolved system with a dominant spheroidal component.
