The galaxy presents as a relatively smooth, elliptical-like structure. Its core region exhibits a high surface brightness, appearing significantly brighter and more concentrated than the surrounding areas. The overall color profile seems to indicate a population of older stars, with the central bulge appearing more yellow. The galaxy extends outwards from the core with decreasing brightness. Based on its apparent roundness, it is potentially closer to a spherical shape, with only a minor deviation suggesting a slightly elongated form. There are no prominent spiral arms or dust lanes visible. Evidence suggests it is not currently undergoing a major merging event, instead showing the possibility of a minor disturbance to its current shape.
