The galaxy appears as a relatively smooth, elliptical-shaped structure. There is a concentrated central bulge, and the light distribution fades gradually outward. The color is predominantly yellowish, suggesting a population of older stars. There are no clearly discernible spiral arms or dust lanes. It appears to be fairly massive. There is no obvious sign of an ongoing major merger, although some minor disturbance cannot be ruled out due to the image quality. Overall, this galaxy seems consistent with an elliptical type with a relatively low rate of star formation.
