The galaxy presents as a single, luminous object, appearing predominantly smooth with a somewhat rounded morphology. Its core exhibits a bright, concentrated emission, transitioning to a dimmer, diffused halo. There is some evidence of a minor disturbance visible as a faint feature to the lower left of the core. The overall color suggests a relatively older stellar population, though some star formation cannot be ruled out. There is no obvious disk structure or spiral arm morphology discernible.
