The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with a highly concentrated central bulge. The overall color appears relatively blue, indicative of the presence of a population of younger, hotter stars, though some redder populations may also be present. There is no distinct spiral structure visible, supporting the elliptical classification. The galaxy is relatively symmetrical and round in shape, with no significant tidal features or major disturbances observed, although some minor asymmetry cannot be ruled out. Based on its red shift, the galaxy is at a considerable distance, making detailed morphological study challenging.
