The galaxy presents a predominantly smooth morphology. The light profile appears concentrated, with a central bulge that dominates the galaxy's overall structure. The shape is elliptical, tending toward a flattened, though not highly elongated, form. A slight asymmetry is noted, potentially indicating minor gravitational disturbance. The overall color suggests an older stellar population, though some regions exhibit bluer hues, potentially indicating pockets of more recent star formation. There are no clearly defined spiral arms or a prominent disk. The galaxy exhibits characteristics consistent with a relatively high mass and a moderate rate of star formation. Evidence suggests the galaxy is in a relatively stable state, with no major ongoing merger events, though some minor disturbances cannot be ruled out.
