The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively featureless. Its core exhibits a high surface brightness, with light gradually diminishing outwards toward the edges. The light distribution suggests an older stellar population dominating, with a color gradient indicating a likely lack of significant ongoing star formation. There is a slight elongation in its shape, leaning towards an 'in between' or intermediate classification, rather than being perfectly spherical or highly elongated. No major disturbances or signs of ongoing merger activity are readily apparent, hinting at a gravitationally settled state. The galaxy's red color suggests that this system is not undergoing much star formation, but instead is made up of older stars.
