The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The central region shows a high degree of luminosity, likely indicative of a significant stellar population density. The overall shape is somewhat elliptical, deviating slightly from a perfect spheroid. Fainter, more diffuse light extends outwards from the central bulge, hinting at a surrounding disk or halo. There are some subtle hints of spiral arm-like features, but they are not sharply defined. The light distribution suggests that this is a relatively evolved galaxy, possibly an intermediate type between a pure elliptical and a spiral. There is a small chance that there is a disturbance in the form of a companion galaxy, but it is too far away to detect.
