The galaxy presents as a moderately bright object with a slightly elliptical morphology. It appears relatively smooth in texture, with a subtle central concentration of light. There is a hint of a disk-like structure, but no prominent spiral arms or bar features are discernible. The overall color suggests a population of older stars, with a relatively red hue. There is no obvious indication of intense star formation regions within the visible portion of the galaxy. The galaxy appears relatively isolated, without any clear signs of a major ongoing merger event, though some minor disturbances are not ruled out. The shape is not perfectly round, but not overly elongated.
