The galaxy presents a generally smooth morphology. It is elliptical, appearing mostly round with slight deviation. The color profile suggests a population of older stars, indicated by the yellow-red hue concentrated toward the galaxy's center. There is very little evidence of dust lanes or spiral arm structures. The galaxy appears quiescent, with a low rate of star formation. No major interactions or mergers are apparent; however, there may be a very slight disturbance in the outer halo. The galaxy’s light is concentrated toward the core, with a diminishing halo.
