The galaxy presents as a relatively smooth, centralized concentration of light, suggesting a spheroid morphology. There is a slight elongation, with the structure appearing more "in between" oval and round. The central region exhibits a yellow-orange hue. This transitions to a more greenish tinge at its outer edges. There are no obvious spiral arms, bar structures, or signs of significant recent merging activity visible in this image, although subtle disturbances cannot be ruled out. Overall, the galaxy seems to be fairly massive with a correspondingly low rate of star formation.
