The galaxy presents a somewhat amorphous morphology, displaying a relatively smooth appearance with some discernible features. Its overall shape is neither perfectly spherical nor highly elongated, leaning more towards an intermediate form. A fraction of the observed light indicates possible disklike qualities. The galaxy exhibits a central bulge with relatively symmetrical light distribution, with an indication of minor disturbances. There are signs of moderate star formation activity occurring within the galaxy. Based on the galaxy's red shift, it is located at a considerable distance. The color indices suggest a moderate presence of both young, blue stars and older, redder stellar populations.
