The galaxy appears to be a large, relatively bright object, characterized by a generally smooth, elliptical morphology. The light distribution is centrally concentrated, with a gradual decline in surface brightness moving outwards. There is a hint of a slight elongation along one axis, but overall the galaxy presents a largely symmetrical form. The galaxy exhibits a yellowish-white hue indicative of an older stellar population, with limited evidence of ongoing star formation. There may be some minor disturbances within the galactic structure. It is estimated to be a high mass galaxy with moderate amounts of star formation.
