The galaxy presents a relatively smooth, elliptical morphology, with a moderate concentration of light towards the center. There is evidence of some disturbance in the galaxy's structure, it does not appear perfectly symmetrical and shows some signs of possible interaction or recent minor merger activity. The object exhibits a moderate degree of roundness, appearing somewhere between perfectly circular and elongated. The color profile suggests an older stellar population, leaning towards redder hues, but there is also a bluish tint suggesting there might be an intermediate amount of star formation. Overall, the galaxy seems to be a fairly massive system, likely undergoing some evolutionary process.
