The galaxy appears to be an elliptical or lenticular system, exhibiting a smooth, centralized light distribution. It appears highly homogenous. Its shape is elongated, displaying an axial ratio that deviates significantly from spherical, leaning towards a cigar-shaped morphology. There is a central bulge that is yellow in color and appears more densely concentrated compared to the outer regions of the galaxy. The extended halo exhibits a blue shift in color around the outer edges, which could suggest the presence of younger stellar populations or recent star formation in these regions, but at a relatively low rate. No clear evidence of spiral arms, dust lanes, or other distinct features commonly associated with spiral galaxies are visible within the system at this resolution. The object does not present any obvious signs of major mergers or significant tidal disturbances, suggesting a relatively undisturbed evolutionary history.
