The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The color profile suggests an older stellar population, exhibiting a yellowish-red hue concentrated towards the center, grading into a fainter, bluish halo extending outwards. There appears to be little to no discernible spiral structure or significant dust lanes. The galaxy appears relatively undisturbed with no obvious signs of major mergers or tidal interactions. Minor disturbances cannot be ruled out with this level of detail. The overall appearance is consistent with an elliptical or lenticular galaxy, with a substantial central bulge. The light distribution appears quite even and symmetrical.
