The galaxy appears as an elongated structure with a relatively smooth, centralized light distribution. The color suggests a mixture of stellar populations, with a somewhat yellowish hue dominating the central region, possibly indicative of older stars. There appears to be some structure present but not clearly organized in terms of spiral arms or a distinct bar. The morphology suggests it is somewhat settled but with subtle perturbations present. Overall, the galaxy appears to be a disk galaxy, possibly in an early stage of a merger or close encounter with another galaxy.
