The galaxy exhibits an elliptical morphology, appearing mostly smooth and spheroidal in shape with little indication of spiral arm structures. It displays a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The color profile suggests a dominant older stellar population, with a yellowish-red hue, indicating lower star formation activity within the galaxy. The galaxy's light is slightly elongated; it is not perfectly circular. There is also some visual evidence of minor disturbances. These disturbances could be caused by interactions with smaller galaxies, internal dynamics, or gravitational effects, however more research will be needed to determine this.
